1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182 183 184 185 186 187 188 189 190 191 192 193 194 195 196 197 198 199 200 201 202 203 204 205 206 207 208 209 210 211 212 213 214 215 216 217 218 219 220 221 222 223 224 225 226 227 228 229 230 231 232 233 234 235 236 237 238 239 240 241 242 243 244 245 246 247 248 249 250 251 252 253 254 255 256 257 258 259 260 261 262 263 264 265 266 267 268 269 270 271 272 273 274 275 276 277 278 279 280 281 282 283 284 285 286 287 288 289 290 291 292 293 294 295 296 297 298 299 300 301 302 303 304 305 306 307 308 309 310 311 312 313 314 315 316 317 318 319 320 321 322 323 324 325 326 327 328 329 330 331 332 333 334 335 336 337 338 339 340 341 342 343 344 345 346 347 348 349 350 351 352 353 354 355 356 357 358 359 360 361 362 363 364 365 366 367 368 369 370 371 372 373 374 375 376 377 378 379 380 381 382 383 384 385 386 387 388 389 390 391 392 393 394 395 396 397 398 399 400 401 402 403 404 405 406 407 408 409 410 411 412 413 414 415 416 417 418 419 420 421 422 423 424 425 426 427 428 429 430 431 432 433 434 435 436 437 438 439 440 441 442 443 444 445 446 447 448 449 450 451 452 453 454 455 456 457 458 459 460 461 462 463 464 465 466 467 468 469 470 471 472 473 474 475 476 477 478 479 480 481 482 483 484 485 486 487 488 489 490 491 492 493 494 495 496 497 498 499 500 501 502 503 504 505 506 507 508 509 510 511 512 513 514 515 516 517 518 519 520 521 522 523 524 525 526 527 528 529 530 531 532 533 534 535 536 537 538 539 540 541 542 543 544 545 546 547 548 549 550 551 552 553 554 555 556 557 558 559 560 561 562 563 564 565 566 567 568 569 570 571 572 573 574 575 576 577 578 579 580 581 582 583 584 585 586 587 588 589 590 591 592 593 594 595 596 597 598 599 600 601 602 603 604 605 606 607 608 609 610 611 612 613 614 615 616 617 618 619 620 621 622 623 624 625 626 627 628 629 630 631 632 633 634 635 636 637 638 639 640 641 642 643 644 645 646 647 648 649 650 651 652 653 654 655 656 657 658 659 660 661 662 663 664 665 666 667 668 669 670 671 672 673 674 675 676 677 678 679 680 681 682 683 684 685 686 687 688 689 690 691 692 693 694 695 696 697 698 699 700 701 702 703 704 705 706 707 708 709 710 711 712 713 714 715 716 717 718 719 720 721 722 723 724 725 726 727 728 729 730 731 732 733 734 735 736 737 738 739 740 741 742 743 744 745 746 747 748 749 750 751 752 753 754 755 756 757 758 759 760 761 762 763 764 765 766 767 768 769 770 771 772 773 774 775 776 777 778 779 780 781 782 783 784 785 786 787 788 789 790 791 792 793 794 795 796 797 798 799 800 801 802 803 804 805 806 807 808 809 810 811 812 813 814 815 816 817 818 819 820 821 822 823 824 825 826 827 828 829 830 831 832 833 834 835 836 837 838 839 840 841 842 843 844 845 846 847 848 849 850 851 852 853 854 855 856 857 858 859 860 861 862 863 864 865 866 867 868 869 870 871 872 873 874 875 876 877 878 879 880 881 882 883 884 885 886 887 888 889 890 891 892 893 894 895 896 897 898 899 900 901 902 903 904 905 906 907 908 909 910 911 912 913 914 915 916 917 918 919 920 921 922 923 924 925 926 927 928 929 930 931 932 933 934 935 936 937 938 939 940 941 942 943 944 945 946 947 948 949 950 951 952 953 954 955 956 957 958 959 960 961 962 963 964 965 966 967 968 969 970 971 972 973 974 975 976 977 978 979 980 981 982 983 984 985 986 987 988 989 990 991 992 993 994 995 996 997 998 999 1000 1001 1002 1003 1004 1005 1006 1007 1008 1009 1010 1011 1012 1013 1014 1015 1016 1017 1018 1019 1020 1021 1022 1023 1024 1025 1026 1027 1028 1029 1030 1031 1032 1033 1034 1035 1036 1037 1038 1039 1040 1041 1042 1043 1044 1045 1046 1047 1048 1049 1050 1051 1052 1053 1054 1055 1056 1057 1058 1059 1060 1061 1062 1063 1064 1065 1066 1067 1068 1069 1070 1071 1072 1073 1074 1075 1076 1077 1078 1079 1080 1081 1082 1083 1084 1085 1086 1087 1088 1089 1090 1091 1092 1093 1094 1095 1096 1097 1098 1099 1100 1101 1102 1103 1104 1105 1106 1107 1108 1109 1110 1111 1112 1113 1114 1115 1116 1117 1118 1119 1120 1121 1122 1123 1124 1125 1126 1127 1128 1129 1130 1131 1132 1133 1134 1135 1136 1137 1138 1139 1140 1141 1142 1143 1144 1145 1146 1147 1148 1149 1150 1151 1152 1153 1154 1155 1156 1157 1158 1159 1160 1161 1162 1163 1164 1165 1166 1167 1168 1169 1170 1171 1172 1173 1174 1175 1176 1177 1178 1179 1180 1181 1182 1183 1184 1185 1186 1187 1188 1189 1190 1191 1192 1193 1194 1195 1196 1197 1198 1199 1200 1201 1202 1203 1204 1205 1206 1207 1208 1209 1210 1211 1212 1213 1214 1215 1216 1217 1218 1219 1220 1221 1222 1223 1224 1225 1226 1227 1228 1229 1230 1231 1232 1233 1234 1235 1236 1237 1238 1239 1240 1241 1242 1243 1244 1245 1246 1247 1248 1249 1250 1251 1252 1253 1254 1255 1256 1257 1258 1259 1260 1261 1262 1263 1264 1265 1266 1267 1268 1269 1270 1271 1272 1273 1274 1275 1276 1277 1278 1279 1280 1281 1282 1283 1284 1285 1286 1287 1288 1289 1290 1291 1292 1293 1294 1295 1296 1297 1298 1299 1300 1301 1302 1303 1304 1305 1306 1307 1308 1309 1310 1311 1312 1313 1314 1315 1316 1317 1318 1319 1320 1321 1322 1323 1324 1325 1326 1327 1328 1329 1330 1331 1332 1333 1334 1335 1336 1337 1338 1339 1340 1341 1342 1343 1344 1345 1346 1347 1348 1349 1350 1351 1352 1353 1354 1355 1356 1357 1358 1359 1360 1361 1362 1363 1364 1365 1366 1367 1368 1369 1370 1371 1372 1373 1374 1375 1376 1377 1378 1379 1380 1381 1382 1383 1384 1385 1386 1387 1388 1389 1390 1391 1392 1393 1394 1395 1396 1397 1398 1399 1400 1401 1402 1403 1404 1405 1406 1407 1408 1409 1410 1411 1412 1413 1414 1415 1416 1417 1418 1419 1420 1421 1422 1423 1424 1425 1426 1427 1428 1429 1430 1431 1432 1433 1434 1435 1436 1437 1438 1439 1440 1441 1442 1443 1444 1445 1446 1447 1448 1449 1450 1451 1452 1453 1454 1455 1456 1457 1458 1459 1460 1461 1462 1463 1464 1465 1466 1467 1468 1469 1470 1471 1472 1473 1474 1475 1476 1477 1478 1479 1480 1481 1482 1483 1484 1485 1486 1487 1488 1489 1490 1491 1492 1493 1494 1495 1496 1497 1498 1499 1500 1501 1502 1503 1504 1505 1506 1507 1508 1509 1510 1511 1512 1513 1514 1515 1516 1517 1518 1519 1520 1521 1522 1523 1524 1525 1526 1527 1528 1529 1530 1531 1532 1533 1534 1535 1536 1537 1538 1539 1540 1541 1542 1543 1544 1545 1546 1547 1548 1549 1550 1551 1552 1553 1554 1555 1556 1557 1558 1559 1560 1561 1562 1563 1564 1565 1566 1567 1568 1569 1570 1571 1572 1573 1574 1575 1576 1577 1578 1579 1580 1581 1582 1583 1584 1585 1586 1587 1588 1589 1590 1591 1592 1593 1594 1595 1596 1597 1598 1599 1600 1601 1602 1603 1604 1605 1606 1607 1608 1609 1610 1611 1612 1613 1614 1615 1616 1617 1618 1619 1620 1621 1622 1623 1624 1625 1626 1627 1628 1629 1630 1631 1632 1633 1634 1635 1636 1637 1638 1639 1640 1641 1642 1643 1644 1645 1646 1647 1648 1649 1650 1651 1652 1653 1654 1655 1656 1657 1658 1659 1660 1661 1662 1663 1664 1665 1666 1667 1668 1669 1670 1671 1672 1673 1674 1675 1676 1677 1678 1679 1680 1681 1682 1683 1684 1685 1686 1687 1688 1689 1690 1691 1692 1693 1694 1695 1696 1697 1698 1699 1700 1701 1702 1703 1704 1705 1706 1707 1708 1709 1710 1711 1712 1713 1714 1715 1716 1717 1718 1719 1720 1721 1722 1723 1724 1725 1726 1727 1728 1729 1730 1731 1732 1733 1734 1735 1736 1737 1738 1739 1740 1741 1742 1743 1744 1745 1746 1747 1748 1749 1750 1751 1752 1753 1754 1755 1756 1757 1758 1759 1760 1761 1762 1763 1764 1765 1766 1767 1768 1769 1770 1771 1772 1773 1774 1775 1776 1777 1778 1779 1780 1781 1782 1783 1784 1785 1786 1787 1788 1789 1790 1791 1792 1793 1794 1795 1796 1797 1798 1799 1800 1801 1802 1803 1804 1805 1806 1807 1808 1809 1810 1811 1812 1813 1814 1815 1816 1817 1818 1819 1820 1821 1822 1823 1824 1825 1826 1827 1828 1829 1830 1831 1832 1833 1834 1835 1836 1837 1838 1839 1840 1841 1842 1843 1844 1845 1846 1847 1848 1849 1850 1851 1852 1853 1854 1855 1856 1857 1858 1859 1860 1861 1862 1863 1864 1865 1866 1867 1868 1869 1870 1871 1872 1873 1874 1875 1876 1877 1878 1879 1880 1881 1882 1883 1884 1885 1886 1887 1888 1889 1890 1891 1892 1893 1894 1895 1896 1897 1898 1899 1900 1901 1902 1903 1904 1905 1906 1907 1908 1909 1910 1911 1912 1913 1914 1915 1916 1917 1918 1919 1920 1921 1922 1923 1924 1925 1926 1927 1928 1929 1930 1931 1932 1933 1934 1935 1936 1937 1938 1939 1940 1941 1942 1943 1944 1945 1946 1947 1948 1949 1950 1951 1952 1953 1954 1955 1956 1957 1958 1959 1960 1961 1962 1963 1964 1965 1966 1967 1968 1969 1970 1971 1972 1973 1974 1975 1976 1977 1978 1979 1980 1981 1982 1983 1984 1985 1986 1987 1988 1989 1990 1991 1992 1993 1994 1995 1996 1997 1998 1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 2020 2021 2022 2023 2024 2025 2026 2027 2028 2029 2030 2031 2032 2033 2034 2035 2036 2037 2038 2039 2040 2041 2042 2043 2044 2045 2046 2047 2048 2049 2050 2051 2052 2053 2054 2055 2056 2057 2058 2059 2060 2061 2062 2063 2064 2065 2066 2067 2068 2069 2070 2071 2072 2073 2074 2075 2076 2077 2078 2079 2080 2081 2082 2083 2084 2085 2086 2087 2088 2089 2090 2091 2092 2093 2094 2095 2096 2097 2098 2099 2100 2101 2102 2103 2104 2105 2106 2107 2108 2109 2110 2111 2112 2113 2114 2115 2116 2117 2118 2119 2120 2121 2122 2123 2124 2125 2126 2127 2128 2129 2130 2131 2132 2133 2134 2135 2136 2137 2138 2139 2140 2141 2142 2143 2144 2145 2146 2147 2148 2149 2150 2151 2152 2153 2154 2155 2156 2157 2158 2159 2160 2161 2162 2163 2164 2165 2166 2167 2168 2169 2170 2171 2172 2173 2174 2175 2176 2177 2178 2179 2180 2181 2182 2183 2184 2185 2186 2187 2188 2189 2190 2191 2192 2193 2194 2195 2196 2197 2198 2199 2200 2201 2202 2203 2204 2205 2206 2207 2208 2209 2210 2211 2212 2213 2214 2215 2216 2217 2218 2219 2220 2221 2222 2223 2224 2225 2226 2227 2228 2229 2230 2231 2232 2233 2234 2235 2236 2237 2238 2239 2240 2241 2242 2243 2244 2245 2246 2247 2248 2249 2250 2251 2252 2253 2254 2255 2256 2257 2258 2259 2260 2261 2262 2263 2264 2265 2266 2267 2268 2269 2270 2271 2272 2273 2274 2275 2276 2277 2278 2279 2280 2281 2282 2283 2284 2285 2286 2287 2288 2289 2290 2291 2292 2293 2294 2295 2296 2297 2298 2299 2300 2301 2302 2303 2304 2305 2306 2307 2308 2309 2310 2311 2312 2313 2314 2315 2316 2317 2318 2319 2320 2321 2322 2323 2324 2325 2326 2327 2328 2329 2330 2331 2332 2333 2334 2335 2336 2337 2338 2339 2340 2341 2342 2343 2344 2345 2346 2347 2348 2349 2350 2351 2352 2353 2354 2355 2356 2357 2358 2359 2360 2361 2362 2363 2364 2365 2366 2367 2368 2369 2370 2371 2372 2373 2374 2375 2376 2377 2378 2379 2380 2381 2382 2383 2384 2385 2386 2387 2388 2389 2390 2391 2392 2393 2394 2395 2396 2397 2398 2399 2400 2401 2402 2403 2404 2405 2406 2407 2408 2409 2410 2411 2412 2413 2414 2415 2416 2417 2418 2419 2420 2421 2422 2423 2424 2425 2426 2427 2428 2429 2430 2431 2432 2433 2434 2435 2436 2437 2438 2439 2440 2441 2442 2443 2444 2445 2446 2447 2448 2449 2450 2451 2452 2453 2454 2455 2456 2457 2458 2459 2460 2461 2462 2463 2464 2465 2466 2467 2468 2469 2470 2471 2472 2473 2474 2475 2476 2477 2478 2479 2480 2481 2482 2483 2484 2485 2486 2487 2488 2489 2490 2491 2492 2493 2494 2495 2496 2497 2498 2499 2500 2501 2502 2503 2504 2505 2506 2507 2508 2509 2510 2511 2512 2513 2514 2515 2516 2517 2518 2519 2520 2521 2522 2523 2524 2525 2526 2527 2528 2529 2530 2531 2532 2533 2534 2535 2536 2537 2538 2539 2540 2541 2542 2543 2544 2545 2546 2547 2548 2549 2550 2551 2552 2553 2554 2555 2556 2557 2558 2559 2560 2561 2562 2563 2564 2565 2566 2567 2568 2569 2570 2571 2572 2573 2574 2575 2576 2577 2578 2579 2580 2581 2582 2583 2584 2585 2586 2587 2588 2589 2590 2591 2592 2593 2594 2595 2596 2597 2598 2599 2600 2601 2602 2603 2604 2605 2606 2607 2608 2609 2610 2611 2612 2613 2614 2615 2616 2617 2618 2619 2620 2621 2622 2623 2624 2625 2626 2627 2628 2629 2630 2631 2632 2633 2634 2635 2636 2637 2638 2639 2640 2641 2642 2643 2644 2645 2646 2647 2648 2649 2650 2651 2652 2653 2654 2655 2656 2657 2658 2659 2660 2661 2662 2663 2664 2665 2666 2667 2668 2669 2670 2671 2672 2673 2674 2675 2676 2677 2678 2679 2680 2681 2682 2683 2684 2685 2686 2687 2688 2689 2690 2691 2692 2693 2694 2695 2696 2697 2698 2699 2700 2701 2702 2703 2704 2705 2706 2707 2708 2709 2710 2711 2712 2713 2714 2715 2716 2717 2718 2719 2720 2721 2722 2723 2724 2725 2726 2727 2728 2729 2730 2731 2732 2733 2734 2735 2736 2737 2738 2739 2740 2741 2742 2743 2744 2745 2746 2747 2748 2749 2750 2751 2752 2753 2754 2755 2756 2757 2758 2759 2760 2761 2762 2763 2764 2765 2766 2767 2768 2769 2770 2771 2772 2773 2774 2775 2776 2777 2778 2779 2780 2781 2782 2783 2784 2785 2786 2787 2788 2789 2790 2791 2792 2793 2794 2795 2796 2797 2798 2799 2800 2801 2802 2803 2804 2805 2806 2807 2808 2809 2810 2811 2812 2813 2814 2815 2816 2817 2818 2819 2820 2821 2822 2823 2824 2825 2826 2827 2828 2829 2830 2831 2832 2833 2834 2835 2836 2837 2838 2839 2840 2841 2842 2843 2844 2845 2846 2847 2848 2849 2850 2851 2852 2853 2854 2855 2856 2857 2858 2859 2860 2861 2862 2863 2864 2865 2866 2867 2868 2869 2870 2871 2872 2873 2874 2875 2876 2877 2878 2879 2880 2881 2882 2883 2884 2885 2886 2887 2888 2889 2890 2891 2892 2893 2894 2895 2896 2897 2898 2899 2900 2901 2902 2903 2904 2905 2906 2907 2908 2909 2910 2911 2912 2913 2914 2915 2916 2917 2918 2919 2920 2921 2922 2923 2924 2925 2926 2927 2928 2929 2930 2931 2932 2933 2934 2935 2936 2937 2938 2939 2940 2941 2942 2943 2944 2945 2946 2947 2948 2949 2950 2951 2952 2953 2954 2955 2956 2957 2958 2959 2960 2961 2962 2963 2964 2965 2966 2967 2968 2969 2970 2971 2972 2973 2974 2975 2976 2977 2978 2979 2980 2981 2982 2983 2984 2985 2986 2987 2988 2989 2990 2991 2992 2993 2994 2995 2996 2997 2998 2999 3000 3001 3002 3003 3004 3005 3006 3007 3008 3009 3010 3011 3012 3013 3014 3015 3016 3017 3018 3019 3020 3021 3022 3023 3024 3025 3026 3027 3028 3029 3030 3031 3032 3033 3034 3035 3036 3037 3038 3039 3040 3041 3042 3043 3044 3045 3046 3047 3048 3049 3050 3051 3052 3053 3054 3055 3056 3057 3058 3059 3060 3061 3062 3063 3064 3065 3066 3067 3068 3069 3070 3071 3072 3073 3074 3075 3076 3077 3078 3079 3080 3081 3082 3083 3084 3085 3086 3087 3088 3089 3090 3091 3092 3093 3094 3095 3096 3097 3098 3099 3100 3101 3102 3103 3104 3105 3106 3107 3108 3109 3110 3111 3112 3113 3114 3115 3116 3117 3118 3119 3120 3121 3122 3123 3124 3125 3126 3127 3128 3129 3130 3131 3132 3133 3134 3135 3136 3137 3138 3139 3140 3141 3142 3143 3144 3145 3146 3147 3148 3149 3150 3151 3152 3153 3154 3155 3156 3157 3158 3159 3160 3161 3162 3163 3164 3165 3166 3167 3168 3169 3170 3171 3172 3173 3174 3175 3176 3177 3178 3179 3180 3181 3182 3183 3184 3185 3186 3187 3188 3189 3190 3191 3192 3193 3194 3195 3196 3197 3198 3199 3200 3201 3202 3203 3204 3205 3206 3207 3208 3209 3210 3211 3212 3213 3214 3215 3216 3217 3218 3219 3220 3221 3222 3223 3224 3225 3226 3227 3228 3229 3230 3231 3232 3233 3234 3235 3236 3237 3238 3239 3240 3241 3242 3243 3244 3245 3246 3247 3248 3249 3250 3251 3252 3253 3254 3255 3256 3257 3258 3259 3260 3261 3262 3263 3264 3265 3266 3267 3268 3269 3270 3271 3272 3273 3274 3275 3276 3277 3278 3279 3280 3281 3282 3283 3284 3285 3286 3287 3288 3289 3290 3291 3292 3293 3294 3295 3296 3297 3298 3299 3300 3301 3302 3303 3304 3305 3306 3307 3308 3309 3310 3311 3312 3313 3314 3315 3316 3317 3318 3319 3320 3321 3322 3323 3324 3325 3326 3327 3328 3329 3330 3331 3332 3333 3334 3335 3336 3337 3338 3339 3340 3341 3342 3343 3344 3345 3346 3347 3348 3349 3350 3351 3352 3353 3354 3355 3356 3357 3358 3359 3360 3361 3362 3363 3364 3365 3366 3367 3368 3369 3370 3371 3372 3373 3374 3375 3376 3377 3378 3379 3380 3381 3382 3383 3384 3385 3386 3387 3388 3389 3390 3391 3392 3393 3394 3395 3396 3397 3398 3399 3400 3401 3402 3403 3404 3405 3406 3407 3408 3409 3410 3411 3412 3413 3414 3415 3416 3417 3418 3419 3420 3421 3422 3423 3424 3425 3426 3427 3428 3429 3430 3431 3432 3433 3434 3435 3436 3437 3438 3439 3440 3441 3442 3443 3444 3445 3446 3447 3448 3449 3450 3451 3452 3453 3454 3455 3456 3457 3458 3459 3460 3461 3462 3463 3464 3465 3466 3467 3468 3469 3470 3471 3472 3473 3474 3475 3476 3477 3478 3479 3480 3481 3482 3483 3484 3485 3486 3487 3488 3489 3490 3491 3492 3493 3494 3495 3496 3497 3498 3499 3500 3501 3502 3503 3504 3505 3506 3507 3508 3509 3510 3511 3512 3513 3514 3515 3516 3517 3518 3519 3520 3521 3522 3523 3524 3525 3526 3527 3528 3529 3530 3531 3532 3533 3534 3535 3536 3537 3538 3539 3540 3541 3542 3543 3544 3545 3546 3547 3548 3549 3550 3551 3552 3553 3554 3555 3556 3557 3558 3559 3560 3561 3562 3563 3564 3565 3566 3567 3568 3569 3570 3571 3572 3573 3574 3575 3576 3577 3578 3579 3580 3581 3582 3583 3584 3585 3586 3587 3588 3589 3590 3591 3592 3593 3594 3595 3596 3597 3598 3599 3600 3601 3602 3603 3604 3605 3606 3607 3608 3609 3610 3611 3612 3613 3614 3615 3616 3617 3618 3619 3620 3621 3622 3623 3624 3625 3626 3627 3628 3629 3630 3631 3632 3633 3634 3635 3636 3637 3638 3639 3640 3641 3642 3643 3644 3645 3646 3647 3648 3649 3650 3651 3652 3653 3654 3655 3656 3657 3658 3659 3660 3661 3662 3663 3664 3665 3666 3667 3668 3669 3670 3671 3672 3673 3674 3675 3676 3677 3678 3679 3680 3681 3682 3683 3684 3685 3686 3687 3688 3689 3690 3691 3692 3693 3694 3695 3696 3697 3698 3699 3700 3701 3702 3703 3704 3705 3706 3707 3708 3709 3710 3711 3712 3713 3714 3715 3716 3717 3718 3719 3720 3721 3722 3723 3724 3725 3726 3727 3728 3729 3730 3731 3732 3733 3734 3735 3736 3737 3738 3739 3740 3741 3742 3743 3744 3745 3746 3747 3748 3749 3750 3751 3752 3753 3754 3755 3756 3757 3758 3759 3760 3761 3762 3763 3764 3765 3766 3767 3768 3769 3770 3771 3772 3773 3774 3775 3776 3777 3778 3779 3780 3781 3782 3783 3784 3785 3786 3787 3788 3789 3790 3791 3792 3793 3794 3795 3796 3797 3798 3799 3800 3801 3802 3803 3804 3805 3806 3807 3808 3809 3810 3811 3812 3813 3814 3815 3816 3817 3818 3819 3820 3821 3822 3823 3824 3825 3826 3827 3828 3829 3830 3831 3832 3833 3834 3835 3836 3837 3838 3839 3840 3841 3842 3843 3844 3845 3846 3847 3848 3849 3850 3851 3852 3853 3854 3855 3856 3857 3858 3859 3860 3861 3862 3863 3864 3865 3866 3867 3868 3869 3870 3871 3872 3873 3874 3875 3876 3877 3878 3879 3880 3881 3882 3883 3884 3885 3886 3887 3888 3889 3890 3891 3892 3893 3894 3895 3896 3897 3898 3899 3900 3901 3902 3903 3904 3905 3906 3907 3908 3909 3910 3911 3912 3913 3914 3915 3916 3917 3918 3919 3920 3921 3922 3923 3924 3925 3926 3927 3928 3929 3930 3931 3932 3933 3934 3935 3936 3937 3938 3939 3940 3941 3942 3943 3944 3945 3946 3947 3948 3949 3950 3951 3952 3953 3954 3955 3956 3957 3958 3959 3960 3961 3962 3963 3964 3965 3966 3967 3968 3969 3970 3971 3972 3973 3974 3975 3976 3977 3978 3979 3980 3981 3982 3983 3984 3985 3986 3987 3988 3989 3990 3991 3992 3993 3994 3995 3996 3997 3998 3999 4000 4001 4002 4003 4004 4005 4006 4007 4008 4009 4010 4011 4012 4013 4014 4015 4016 4017 4018 4019 4020 4021 4022 4023 4024 4025 4026 4027 4028 4029 4030 4031 4032 4033 4034 4035 4036 4037 4038 4039 4040 4041 4042 4043 4044 4045 4046 4047 4048 4049 4050 4051 4052 4053 4054 4055 4056 4057 4058 4059 4060 4061 4062 4063 4064 4065 4066 4067 4068 4069 4070 4071 4072 4073 4074 4075 4076 4077 4078 4079 4080 4081 4082 4083 4084 4085 4086 4087 4088 4089 4090 4091 4092 4093 4094 4095 4096 4097 4098 4099 4100 4101 4102 4103 4104 4105 4106 4107 4108 4109 4110 4111 4112 4113 4114 4115 4116 4117 4118 4119 4120 4121 4122 4123 4124 4125 4126 4127 4128 4129 4130 4131 4132 4133 4134 4135 4136 4137 4138 4139 4140 4141 4142 4143 4144 4145 4146 4147 4148 4149 4150 4151 4152 4153 4154 4155 4156 4157 4158 4159 4160 4161 4162 4163 4164 4165 4166 4167 4168 4169 4170 4171 4172 4173 4174 4175 4176 4177 4178 4179 4180 4181 4182 4183 4184 4185 4186 4187 4188 4189 4190 4191 4192 4193 4194 4195 4196 4197 4198 4199 4200 4201 4202 4203 4204 4205 4206 4207 4208 4209 4210 4211 4212 4213 4214 4215 4216 4217 4218 4219 4220 4221 4222 4223 4224 4225 4226 4227 4228 4229 4230 4231 4232 4233 4234 4235 4236 4237 4238 4239 4240 4241 4242 4243 4244 4245 4246 4247 4248 4249 4250 4251 4252 4253 4254 4255 4256 4257 4258 4259 4260 4261 4262 4263 4264 4265 4266 4267 4268 4269 4270 4271 4272 4273 4274 4275 4276 4277 4278 4279 4280 4281 4282 4283 4284 4285 4286 4287 4288 4289 4290 4291 4292 4293 4294 4295 4296 4297 4298 4299 4300 4301 4302 4303 4304 4305 4306 4307 4308 4309 4310 4311 4312 4313 4314 4315 4316 4317 4318 4319 4320 4321 4322 4323 4324 4325 4326 4327 4328 4329 4330 4331 4332 4333 4334 4335 4336 4337 4338 4339 4340 4341 4342 4343 4344 4345 4346 4347 4348 4349 4350 4351 4352 4353 4354 4355 4356 4357 4358 4359 4360 4361 4362 4363 4364 4365 4366 4367 4368 4369 4370 4371 4372 4373 4374 4375 4376 4377 4378 4379 4380 4381 4382 4383 4384 4385 4386 4387 4388 4389 4390 4391 4392 4393 4394 4395 4396 4397 4398 4399 4400 4401 4402 4403 4404 4405 4406 4407 4408 4409 4410 4411 4412 4413 4414 4415 4416 4417 4418 4419 4420 4421 4422 4423 4424 4425 4426 4427 4428 4429 4430 4431 4432 4433 4434 4435 4436 4437 4438 4439 4440 4441 4442 4443 4444 4445 4446 4447 4448 4449 4450 4451 4452 4453 4454 4455 4456 4457 4458 4459 4460 4461 4462 4463 4464 4465 4466 4467 4468 4469 4470 4471 4472 4473 4474 4475 4476 4477 4478 4479 4480 4481 4482 4483 4484 4485 4486 4487 4488 4489 4490 4491 4492 4493 4494 4495 4496 4497 4498 4499 4500 4501 4502 4503 4504 4505 4506 4507 4508 4509 4510 4511 4512 4513 4514 4515 4516 4517 4518 4519 4520 4521 4522 4523 4524 4525 4526 4527 4528 4529 4530 4531 4532 4533 4534 4535 4536 4537 4538 4539 4540 4541 4542 4543 4544 4545 4546 4547 4548 4549 4550 4551 4552 4553 4554 4555 4556 4557 4558 4559 4560 4561 4562 4563 4564 4565 4566 4567 4568 4569 4570 4571 4572 4573 4574 4575 4576 4577 4578 4579 4580 4581 4582 4583 4584 4585 4586 4587 4588 4589 4590 4591 4592 4593 4594 4595 4596 4597 4598 4599 4600 4601 4602 4603 4604 4605 4606 4607 4608 4609 4610 4611 4612 4613 4614 4615 4616 4617 4618 4619 4620 4621 4622 4623 4624 4625 4626 4627 4628 4629 4630 4631 4632 4633 4634 4635 4636 4637 4638 4639 4640 4641 4642 4643 4644 4645 4646 4647 4648 4649 4650 4651 4652 4653 4654 4655 4656 4657 4658 4659 4660 4661 4662 4663 4664 4665 4666 4667 4668 4669 4670 4671 4672 4673 4674 4675 4676 4677 4678 4679 4680 4681 4682 4683 4684 4685 4686 4687 4688 4689 4690 4691 4692 4693 4694 4695 4696 4697 4698 4699 4700 4701 4702 4703 4704 4705 4706 4707 4708 4709 4710 4711 4712 4713 4714 4715 4716 4717 4718 4719 4720 4721 4722 4723 4724 4725 4726 4727 4728 4729 4730 4731 4732 4733 4734 4735 4736 4737 4738 4739 4740 4741 4742 4743 4744 4745 4746 4747 4748 4749 4750 4751 4752 4753 4754 4755 4756 4757 4758 4759 4760 4761 4762 4763 4764 4765 4766 4767 4768 4769 4770 4771 4772 4773 4774 4775 4776 4777 4778 4779 4780 4781 4782 4783 4784 4785 4786 4787 4788 4789 4790 4791 4792 4793 4794 4795 4796 4797 4798 4799 4800 4801 4802 4803 4804 4805 4806 4807 4808 4809 4810 4811 4812 4813 4814 4815 4816 4817 4818 4819 4820 4821 4822 4823 4824 4825 4826 4827 4828 4829 4830 4831 4832 4833 4834 4835 4836 4837 4838 4839 4840 4841 4842 4843 4844 4845 4846 4847 4848 4849 4850 4851 4852 4853 4854 4855 4856 4857 4858 4859 4860 4861 4862 4863 4864 4865 4866 4867 4868 4869 4870 4871 4872 4873 4874 4875 4876 4877 4878 4879 4880 4881 4882 4883 4884 4885 4886 4887 4888 4889 4890 4891 4892 4893 4894 4895 4896 4897 4898 4899 4900 4901 4902 4903 4904 4905 4906 4907 4908 4909 4910 4911 4912 4913 4914 4915 4916 4917 4918 4919 4920 4921 4922 4923 4924 4925 4926 4927 4928 4929 4930 4931 4932 4933 4934 4935 4936 4937 4938 4939 4940 4941 4942 4943 4944 4945 4946 4947 4948 4949 4950 4951 4952 4953 4954 4955 4956 4957 4958 4959 4960 4961 4962 4963 4964 4965 4966 4967 4968 4969 4970 4971 4972 4973 4974 4975 4976 4977 4978 4979 4980 4981 4982 4983 4984 4985 4986 4987 4988 4989 4990 4991 4992 4993 4994 4995 4996 4997 4998 4999 5000 5001 5002 5003 5004 5005 5006 5007 5008 5009 5010 5011 5012 5013 5014 5015 5016 5017 5018 5019 5020 5021 5022 5023 5024 5025 5026 5027 5028 5029 5030 5031 5032 5033 5034 5035 5036 5037 5038 5039 5040 5041 5042 5043 5044 5045 5046 5047 5048 5049 5050 5051 5052 5053 5054 5055 5056 5057 5058 5059 5060 5061 5062 5063 5064 5065 5066 5067 5068 5069 5070 5071 5072 5073 5074 5075 5076 5077 5078 5079 5080 5081 5082 5083 5084 5085 5086 5087 5088 5089 5090 5091 5092 5093 5094 5095 5096 5097 5098 5099 5100 5101 5102 5103 5104 5105 5106 5107 5108 5109 5110 5111 5112 5113 5114 5115 5116 5117 5118 5119 5120 5121 5122 5123 5124 5125 5126 5127 5128 5129 5130 5131 5132 5133 5134 5135 5136 5137 5138 5139 5140 5141 5142 5143 5144 5145 5146 5147 5148 5149 5150 5151 5152 5153 5154 5155 5156 5157 5158 5159 5160 5161 5162 5163 5164 5165 5166 5167 5168 5169 5170 5171 5172 5173 5174 5175 5176 5177 5178 5179 5180 5181 5182 5183 5184 5185 5186 5187 5188 5189 5190 5191 5192 5193 5194 5195 5196 5197 5198 5199 5200 5201 5202 5203 5204 5205 5206 5207 5208 5209 5210 5211 5212 5213 5214 5215 5216 5217 5218 5219 5220 5221 5222 5223 5224 5225 5226 5227 5228 5229 5230 5231 5232 5233 5234 5235 5236 5237 5238 5239 5240 5241 5242 5243 5244 5245 5246 5247 5248 5249 5250 5251 5252 5253 5254 5255 5256 5257 5258 5259 5260 5261 5262 5263 5264 5265 5266 5267 5268 5269 5270 5271 5272 5273 5274 5275 5276 5277 5278 5279 5280 5281 5282 5283 5284 5285 5286 5287 5288 5289 5290 5291 5292 5293 5294 5295 5296 5297 5298 5299 5300 5301 5302 5303 5304 5305 5306 5307 5308 5309 5310 5311 5312 5313 5314 5315 5316 5317 5318 5319 5320 5321 5322 5323 5324 5325 5326 5327 5328 5329 5330 5331 5332 5333 5334 5335 5336 5337 5338 5339 5340 5341 5342 5343 5344 5345 5346 5347 5348 5349 5350 5351 5352 5353 5354 5355 5356 5357 5358 5359 5360 5361 5362 5363 5364 5365 5366 5367 5368 5369 5370 5371 5372 5373 5374 5375 5376 5377 5378 5379 5380 5381 5382 5383 5384 5385 5386 5387 5388 5389 5390 5391 5392 5393 5394 5395 5396 5397 5398 5399 5400 5401 5402 5403 5404 5405 5406 5407 5408 5409 5410 5411 5412 5413 5414 5415 5416 5417 5418 5419 5420 5421 5422 5423 5424 5425 5426 5427 5428 5429 5430 5431 5432 5433 5434 5435 5436 5437 5438 5439 5440 5441 5442 5443 5444 5445 5446 5447 5448 5449 5450 5451 5452 5453 5454 5455 5456 5457 5458 5459 5460 5461 5462 5463 5464 5465 5466 5467 5468 5469 5470 5471 5472 5473 5474 5475 5476 5477 5478 5479 5480 5481 5482 5483 5484 5485 5486 5487 5488 5489 5490 5491 5492 5493 5494 5495 5496 5497 5498 5499 5500 5501 5502 5503 5504 5505 5506 5507 5508 5509 5510 5511 5512 5513 5514 5515 5516 5517 5518 5519 5520 5521 5522 5523 5524 5525 5526 5527 5528 5529 5530 5531 5532 5533 5534 5535 5536 5537 5538 5539 5540 5541 5542 5543 5544 5545 5546 5547 5548 5549 5550 5551 5552 5553 5554 5555 5556 5557 5558 5559 5560 5561 5562 5563 5564 5565 5566 5567 5568 5569 5570 5571 5572 5573 5574 5575 5576 5577 5578 5579 5580 5581 5582 5583 5584 5585 5586 5587 5588 5589 5590 5591 5592 5593 5594 5595 5596 5597 5598 5599 5600 5601 5602 5603 5604 5605 5606 5607 5608 5609 5610 5611 5612 5613 5614 5615 5616 5617 5618 5619 5620 5621 5622 5623 5624 5625 5626 5627 5628 5629 5630 5631 5632 5633 5634 5635 5636 5637 5638 5639 5640 5641 5642 5643 5644 5645 5646 5647 5648 5649 5650 5651 5652 5653 5654 5655 5656 5657 5658 5659 5660 5661 5662 5663 5664 5665 5666 5667 5668 5669 5670 5671 5672 5673 5674 5675 5676 5677 5678 5679 5680 5681 5682 5683 5684 5685 5686 5687 5688 5689 5690 5691 5692 5693 5694 5695 5696 5697 5698 5699 5700 5701 5702 5703 5704 5705 5706 5707 5708 5709 5710 5711 5712 5713 5714 5715 5716 5717 5718 5719 5720 5721 5722 5723 5724 5725 5726 5727 5728 5729 5730 5731 5732 5733 5734 5735 5736 5737 5738 5739 5740 5741 5742 5743 5744 5745 5746 5747 5748 5749 5750 5751 5752 5753 5754 5755 5756 5757 5758 5759 5760 5761 5762 5763 5764 5765 5766 5767 5768 5769 5770 5771 5772 5773 5774 5775 5776 5777 5778 5779 5780 5781 5782 5783 5784 5785 5786 5787 5788 5789 5790 5791 5792 5793 5794 5795 5796 5797 5798 5799 5800 5801 5802 5803 5804 5805 5806 5807 5808 5809 5810 5811 5812 5813 5814 5815 5816 5817 5818 5819 5820 5821 5822 5823 5824 5825 5826 5827 5828 5829 5830 5831 5832 5833 5834 5835 5836 5837 5838 5839 5840 5841 5842 5843 5844 5845 5846 5847 5848 5849 5850 5851 5852 5853 5854 5855 5856 5857 5858 5859 5860 5861 5862 5863 5864 5865 5866 5867 5868 5869 5870 5871 5872 5873 5874 5875 5876 5877 5878 5879 5880 5881 5882 5883 5884 5885 5886 5887 5888 5889 5890 5891 5892 5893 5894 5895 5896 5897 5898 5899 5900 5901 5902 5903 5904 5905 5906 5907 5908 5909 5910 5911 5912 5913 5914 5915 5916 5917 5918 5919 5920 5921 5922 5923 5924 5925 5926 5927 5928 5929 5930 5931 5932 5933 5934 5935 5936 5937 5938 5939 5940 5941 5942 5943 5944 5945 5946 5947 5948 5949 5950 5951 5952 5953 5954 5955 5956 5957 5958 5959 5960 5961 5962 5963 5964 5965 5966 5967 5968 5969 5970 5971 5972 5973 5974 5975 5976 5977 5978 5979 5980 5981 5982 5983 5984 5985 5986 5987 5988 5989 5990 5991 5992 5993 5994 5995 5996 5997 5998 5999 6000 6001 6002 6003 6004 6005 6006 6007 6008 6009 6010 6011 6012 6013 6014 6015 6016 6017 6018 6019 6020 6021 6022 6023 6024 6025 6026 6027 6028 6029 6030 6031 6032 6033 6034 6035 6036 6037 6038 6039 6040 6041 6042 6043 6044 6045 6046 6047 6048 6049 6050 6051 6052 6053 6054 6055 6056 6057 6058 6059 6060 6061 6062 6063 6064 6065 6066 6067 6068 6069 6070 6071 6072 6073 6074 6075 6076 6077 6078 6079 6080 6081 6082 6083 6084 6085 6086 6087 6088 6089 6090 6091 6092 6093 6094 6095 6096 6097 6098 6099 6100 6101 6102 6103 6104 6105 6106 6107 6108 6109 6110 6111 6112 6113 6114 6115 6116 6117 6118 6119 6120 6121 6122 6123 6124 6125 6126 6127 6128 6129 6130 6131 6132 6133 6134 6135 6136 6137 6138 6139 6140 6141 6142 6143 6144 6145 6146 6147 6148 6149 6150 6151 6152 6153 6154 6155 6156 6157 6158 6159 6160 6161 6162 6163 6164 6165 6166 6167 6168 6169 6170 6171 6172 6173 6174 6175 6176 6177 6178 6179 6180 6181 6182 6183 6184 6185 6186 6187 6188 6189 6190 6191 6192 6193 6194 6195 6196 6197 6198 6199 6200 6201 6202 6203 6204 6205 6206 6207 6208 6209 6210 6211 6212 6213 6214 6215 6216 6217 6218 6219 6220 6221 6222 6223 6224 6225 6226 6227 6228 6229 6230 6231 6232 6233 6234 6235 6236 6237 6238 6239 6240 6241 6242 6243 6244 6245 6246 6247 6248 6249 6250 6251 6252 6253 6254 6255 6256 6257 6258 6259 6260 6261 6262 6263 6264 6265 6266 6267 6268 6269 6270 6271 6272 6273 6274 6275 6276 6277 6278 6279 6280 6281 6282 6283 6284 6285 6286 6287 6288 6289 6290 6291 6292 6293 6294 6295 6296 6297 6298 6299 6300 6301 6302 6303 6304 6305 6306 6307 6308 6309 6310 6311 6312 6313 6314 6315 6316 6317 6318 6319 6320 6321 6322 6323 6324 6325 6326 6327 6328 6329 6330 6331 6332 6333 6334 6335 6336 6337 6338 6339 6340 6341 6342 6343 6344 6345 6346 6347 6348 6349 6350 6351 6352 6353 6354 6355 6356 6357 6358 6359 6360 6361 6362 6363 6364 6365 6366 6367 6368 6369 6370 6371 6372 6373 6374 6375 6376 6377 6378 6379 6380 6381 6382 6383 6384 6385 6386 6387 6388 6389 6390 6391 6392 6393 6394 6395 6396 6397 6398 6399 6400 6401 6402 6403 6404 6405 6406 6407 6408 6409 6410 6411 6412 6413 6414 6415 6416 6417 6418 6419 6420 6421 6422 6423 6424 6425 6426 6427 6428 6429 6430 6431 6432 6433 6434 6435 6436 6437 6438 6439 6440 6441 6442 6443 6444 6445 6446 6447 6448 6449 6450 6451 6452 6453 6454 6455 6456 6457 6458 6459 6460 6461 6462 6463 6464 6465 6466 6467 6468 6469 6470 6471 6472 6473 6474 6475 6476 6477 6478 6479 6480 6481 6482 6483 6484 6485 6486 6487 6488 6489 6490 6491 6492 6493 6494 6495 6496 6497 6498 6499 6500 6501 6502 6503 6504 6505 6506 6507 6508 6509 6510 6511 6512 6513 6514 6515 6516 6517 6518 6519 6520 6521 6522 6523 6524 6525 6526 6527 6528 6529 6530 6531 6532 6533 6534 6535 6536 6537 6538 6539 6540 6541 6542 6543 6544 6545 6546 6547 6548 6549 6550 6551 6552 6553 6554 6555 6556 6557 6558 6559 6560 6561 6562 6563 6564 6565 6566 6567 6568 6569 6570 6571 6572 6573 6574 6575 6576 6577 6578 6579 6580 6581 6582 6583 6584 6585 6586 6587 6588 6589 6590 6591 6592 6593 6594 6595 6596 6597 6598 6599 6600 6601 6602 6603 6604 6605 6606 6607 6608 6609 6610 6611 6612 6613 6614 6615 6616 6617 6618 6619 6620 6621 6622 6623 6624 6625 6626 6627 6628 6629 6630 6631 6632 6633 6634 6635 6636 6637 6638 6639 6640 6641 6642 6643 6644 6645 6646 6647 6648 6649 6650 6651 6652 6653 6654 6655 6656 6657 6658 6659 6660 6661 6662 6663 6664 6665 6666 6667 6668 6669 6670 6671 6672 6673 6674 6675 6676 6677 6678 6679 6680 6681 6682 6683 6684 6685 6686 6687 6688 6689 6690 6691 6692 6693 6694 6695 6696 6697 6698 6699 6700 6701 6702 6703 6704 6705 6706 6707 6708 6709 6710 6711 6712 6713 6714 6715 6716 6717 6718 6719 6720 6721 6722 6723 6724 6725 6726 6727 6728 6729 6730 6731 6732 6733 6734 6735 6736 6737 6738 6739 6740 6741 6742 6743 6744 6745 6746 6747 6748 6749 6750 6751 6752 6753 6754 6755 6756 6757 6758 6759 6760 6761 6762 6763 6764 6765 6766 6767 6768 6769 6770 6771 6772 6773 6774 6775 6776 6777 6778 6779 6780 6781 6782 6783 6784 6785 6786 6787 6788 6789 6790 6791 6792 6793 6794 6795 6796 6797 6798 6799 6800 6801 6802 6803 6804 6805 6806 6807 6808 6809 6810 6811 6812 6813 6814 6815 6816 6817 6818 6819 6820 6821 6822 6823 6824 6825 6826 6827 6828 6829 6830 6831 6832 6833 6834 6835 6836 6837 6838 6839 6840 6841 6842 6843 6844 6845 6846 6847 6848 6849 6850 6851 6852 6853 6854 6855 6856 6857 6858 6859 6860 6861 6862 6863 6864 6865 6866 6867 6868 6869 6870 6871 6872 6873 6874 6875 6876 6877 6878 6879 6880 6881 6882 6883 6884 6885 6886 6887 6888 6889 6890 6891 6892 6893 6894 6895 6896 6897 6898 6899 6900 6901 6902 6903 6904 6905 6906 6907 6908 6909 6910 6911 6912 6913 6914 6915 6916 6917 6918 6919 6920 6921 6922 6923 6924 6925 6926 6927 6928 6929 6930 6931 6932 6933 6934 6935 6936 6937 6938 6939 6940 6941 6942 6943 6944 6945 6946 6947 6948 6949 6950 6951 6952 6953 6954 6955 6956 6957 6958 6959 6960 6961 6962 6963 6964 6965 6966 6967 6968 6969 6970 6971 6972 6973 6974 6975 6976 6977 6978 6979 6980 6981 6982 6983 6984 6985 6986 6987 6988 6989 6990 6991 6992 6993 6994 6995 6996 6997 6998 6999 7000 7001 7002 7003 7004 7005 7006 7007 7008 7009 7010 7011 7012 7013 7014 7015 7016 7017 7018 7019 7020 7021 7022 7023 7024 7025 7026 7027 7028 7029 7030 7031 7032 7033 7034 7035 7036 7037 7038 7039 7040 7041 7042 7043 7044 7045 7046 7047 7048 7049 7050 7051 7052 7053 7054 7055 7056 7057 7058 7059 7060 7061 7062 7063 7064 7065 7066 7067 7068 7069 7070 7071 7072 7073 7074 7075 7076 7077 7078 7079 7080 7081 7082 7083 7084 7085 7086 7087 7088 7089 7090 7091 7092 7093 7094 7095 7096 7097 7098 7099 7100 7101 7102 7103 7104 7105 7106 7107 7108 7109 7110 7111 7112 7113 7114 7115 7116 7117 7118 7119 7120 7121 7122 7123 7124 7125 7126 7127 7128 7129 7130 7131 7132 7133 7134 7135 7136 7137 7138 7139 7140 7141 7142 7143 7144 7145 7146 7147 7148 7149 7150 7151 7152 7153 7154 7155 7156 7157 7158 7159 7160 7161 7162 7163 7164 7165 7166 7167 7168 7169 7170 7171 7172 7173 7174 7175 7176 7177 7178 7179 7180 7181 7182 7183 7184 7185 7186 7187 7188 7189 7190 7191 7192 7193 7194 7195 7196 7197 7198 7199 7200 7201 7202 7203 7204 7205 7206 7207 7208 7209 7210 7211 7212 7213 7214 7215 7216 7217 7218 7219 7220 7221 7222 7223 7224 7225 7226 7227 7228 7229 7230 7231 7232 7233 7234 7235 7236 7237 7238 7239 7240 7241 7242 7243 7244 7245 7246 7247 7248 7249 7250 7251 7252 7253 7254 7255 7256 7257 7258 7259 7260 7261 7262 7263 7264 7265 7266 7267 7268 7269 7270 7271 7272 7273 7274 7275 7276 7277 7278 7279 7280 7281 7282 7283 7284 7285 7286 7287 7288 7289 7290 7291 7292 7293 7294 7295 7296 7297 7298 7299 7300 7301 7302 7303 7304 7305 7306 7307 7308 7309 7310 7311 7312 7313 7314 7315 7316 7317 7318 7319 7320 7321 7322 7323 7324 7325 7326 7327 7328 7329 7330 7331 7332 7333 7334 7335 7336 7337 7338 7339 7340 7341 7342 7343 7344 7345 7346 7347 7348 7349 7350 7351 7352 7353 7354 7355 7356 7357 7358 7359 7360 7361 7362 7363 7364 7365 7366 7367 7368 7369 7370 7371 7372 7373 7374 7375 7376 7377 7378 7379 7380 7381 7382 7383 7384 7385 7386 7387 7388 7389 7390 7391 7392 7393 7394 7395 7396 7397 7398 7399 7400 7401 7402 7403 7404 7405 7406 7407 7408 7409 7410 7411 7412 7413 7414 7415 7416 7417 7418 7419 7420 7421 7422 7423 7424 7425 7426 7427 7428 7429 7430 7431 7432 7433 7434 7435 7436 7437 7438 7439 7440 7441 7442 7443 7444 7445 7446 7447 7448 7449 7450 7451 7452 7453 7454 7455 7456 7457 7458 7459 7460 7461 7462 7463 7464 7465 7466 7467 7468 7469 7470 7471 7472 7473 7474 7475 7476 7477 7478 7479 7480 7481 7482 7483 7484 7485 7486 7487 7488 7489 7490 7491 7492 7493 7494 7495 7496 7497 7498 7499 7500 7501 7502 7503 7504 7505 7506 7507 7508 7509 7510 7511 7512 7513 7514 7515 7516 7517 7518 7519 7520 7521 7522 7523 7524 7525 7526 7527 7528 7529 7530 7531 7532 7533 7534 7535 7536 7537 7538 7539 7540 7541 7542 7543 7544 7545 7546 7547 7548 7549 7550 7551 7552 7553 7554 7555 7556 7557 7558 7559 7560 7561 7562 7563 7564 7565 7566 7567 7568 7569 7570 7571 7572 7573 7574 7575 7576 7577 7578 7579 7580 7581 7582 7583 7584 7585 7586 7587 7588 7589 7590 7591 7592 7593 7594 7595 7596 7597 7598 7599 7600 7601 7602 7603 7604 7605 7606 7607 7608 7609 7610 7611 7612 7613 7614 7615 7616 7617 7618 7619 7620 7621 7622 7623 7624 7625 7626 7627 7628 7629 7630 7631 7632 7633 7634 7635 7636 7637 7638 7639 7640 7641 7642 7643 7644 7645 7646 7647 7648 7649 7650 7651 7652 7653 7654 7655 7656 7657 7658 7659 7660 7661 7662 7663 7664 7665 7666 7667 7668 7669 7670 7671 7672 7673 7674 7675 7676 7677 7678 7679 7680 7681 7682 7683 7684 7685 7686 7687 7688 7689 7690 7691 7692 7693 7694 7695 7696 7697 7698 7699 7700 7701 7702 7703 7704 7705 7706 7707 7708 7709 7710 7711 7712 7713 7714 7715 7716 7717 7718 7719 7720 7721 7722 7723 7724 7725 7726 7727 7728 7729 7730 7731 7732 7733 7734 7735 7736 7737 7738 7739 7740 7741 7742 7743 7744 7745 7746 7747 7748 7749 7750 7751 7752 7753 7754 7755 7756 7757 7758 7759 7760 7761 7762 7763 7764 7765 7766 7767 7768 7769 7770 7771 7772 7773 7774 7775 7776 7777 7778 7779 7780 7781 7782 7783 7784 7785 7786 7787 7788 7789 7790 7791 7792 7793 7794 7795 7796 7797 7798 7799 7800 7801 7802 7803 7804 7805 7806 7807 7808 7809 7810 7811 7812 7813 7814 7815 7816 7817 7818 7819 7820 7821 7822 7823 7824 7825 7826 7827 7828 7829 7830 7831 7832 7833 7834 7835 7836 7837 7838 7839 7840 7841 7842 7843 7844 7845 7846 7847 7848 7849 7850 7851 7852 7853 7854 7855 7856 7857 7858 7859 7860 7861 7862 7863 7864 7865 7866 7867 7868 7869 7870 7871 7872 7873 7874 7875 7876 7877 7878 7879 7880 7881 7882 7883 7884 7885 7886 7887 7888 7889 7890 7891 7892 7893 7894 7895 7896 7897 7898 7899 7900 7901 7902 7903 7904 7905 7906 7907 7908 7909 7910 7911 7912 7913 7914 7915 7916 7917 7918 7919 7920 7921 7922 7923 7924 7925 7926 7927 7928 7929 7930 7931 7932 7933 7934 7935 7936 7937 7938 7939 7940 7941 7942 7943 7944 7945 7946 7947 7948 7949 7950 7951 7952 7953 7954 7955 7956 7957 7958 7959 7960 7961 7962 7963 7964 7965 7966 7967 7968 7969 7970 7971 7972 7973 7974 7975 7976 7977 7978 7979 7980 7981 7982 7983 7984 7985 7986 7987 7988 7989 7990 7991 7992 7993 7994 7995 7996 7997 7998 7999 8000 8001 8002 8003 8004 8005 8006 8007 8008 8009 8010 8011 8012 8013 8014 8015 8016 8017 8018 8019 8020 8021 8022 8023 8024 8025 8026 8027 8028 8029 8030 8031 8032 8033 8034 8035 8036 8037 8038 8039 8040 8041 8042 8043 8044 8045 8046 8047 8048 8049 8050 8051 8052 8053 8054 8055 8056 8057 8058 8059 8060 8061 8062 8063 8064 8065 8066 8067 8068 8069 8070 8071 8072 8073 8074 8075 8076 8077 8078 8079 8080 8081 8082 8083 8084 8085 8086 8087 8088 8089 8090 8091 8092 8093 8094 8095 8096 8097 8098 8099 8100 8101 8102 8103 8104 8105 8106 8107 8108 8109 8110 8111 8112 8113 8114 8115 8116 8117 8118 8119 8120 8121 8122 8123 8124 8125 8126 8127 8128 8129 8130 8131 8132 8133 8134 8135 8136 8137 8138 8139 8140 8141 8142 8143 8144 8145 8146 8147 8148 8149 8150 8151 8152 8153 8154 8155 8156 8157 8158 8159 8160 8161 8162 8163 8164 8165 8166 8167 8168 8169 8170 8171 8172 8173 8174 8175 8176 8177 8178 8179 8180 8181 8182 8183 8184 8185 8186 8187 8188 8189 8190 8191 8192 8193 8194 8195 8196 8197 8198 8199 8200 8201 8202 8203 8204 8205 8206 8207 8208 8209 8210 8211 8212 8213 8214 8215 8216 8217 8218 8219 8220 8221 8222 8223 8224 8225 8226 8227 8228 8229 8230 8231 8232 8233 8234 8235 8236 8237 8238 8239 8240 8241 8242 8243 8244 8245 8246 8247 8248 8249 8250 8251 8252 8253 8254 8255 8256 8257 8258 8259 8260 8261 8262 8263 8264 8265 8266 8267 8268 8269 8270 8271 8272 8273 8274 8275 8276 8277 8278 8279 8280 8281 8282 8283 8284 8285 8286 8287 8288 8289 8290 8291 8292 8293 8294 8295 8296 8297 8298 8299 8300 8301 8302 8303 8304 8305 8306 8307 8308 8309 8310 8311 8312 8313 8314 8315 8316 8317 8318 8319 8320 8321 8322 8323 8324 8325 8326 8327 8328 8329 8330 8331 8332 8333 8334 8335 8336 8337 8338 8339 8340 8341 8342 8343 8344 8345 8346 8347 8348 8349 8350 8351 8352 8353 8354 8355 8356 8357 8358 8359 8360 8361 8362 8363 8364 8365 8366 8367 8368 8369 8370 8371 8372 8373 8374 8375 8376 8377 8378 8379 8380 8381 8382 8383 8384 8385 8386 8387 8388 8389 8390 8391 8392 8393 8394 8395 8396 8397 8398 8399 8400 8401 8402 8403 8404 8405 8406 8407 8408 8409 8410 8411 8412 8413 8414 8415 8416 8417 8418 8419 8420 8421 8422 8423 8424 8425 8426 8427 8428 8429 8430 8431 8432 8433 8434 8435 8436 8437 8438 8439 8440 8441 8442 8443 8444 8445 8446 8447 8448 8449 8450 8451 8452 8453 8454 8455 8456 8457 8458 8459 8460 8461 8462 8463 8464 8465 8466 8467 8468 8469 8470 8471 8472 8473 8474 8475 8476 8477 8478 8479 8480 8481 8482 8483 8484 8485 8486 8487 8488 8489 8490 8491 8492 8493 8494 8495 8496 8497 8498 8499 8500 8501 8502 8503 8504 8505 8506 8507 8508 8509 8510 8511 8512 8513 8514 8515 8516 8517 8518 8519 8520 8521 8522 8523 8524 8525 8526 8527 8528 8529 8530 8531 8532 8533 8534 8535 8536 8537 8538 8539 8540 8541 8542 8543 8544 8545 8546 8547 8548 8549 8550 8551 8552 8553 8554 8555 8556 8557 8558 8559 8560 8561 8562 8563 8564 8565 8566 8567 8568 8569 8570 8571 8572 8573 8574 8575 8576 8577 8578 8579 8580 8581 8582 8583 8584 8585 8586 8587 8588 8589 8590 8591 8592 8593 8594 8595 8596 8597 8598 8599 8600 8601 8602 8603 8604 8605 8606 8607 8608 8609 8610 8611 8612 8613 8614 8615 8616 8617 8618 8619 8620 8621 8622 8623 8624 8625 8626 8627 8628 8629 8630 8631 8632 8633 8634 8635 8636 8637 8638 8639 8640 8641 8642 8643 8644 8645 8646 8647 8648 8649 8650 8651 8652 8653 8654 8655 8656 8657 8658 8659 8660 8661 8662 8663 8664 8665 8666 8667 8668 8669 8670 8671 8672 8673 8674 8675 8676 8677 8678 8679 8680 8681 8682 8683 8684 8685 8686 8687 8688 8689 8690 8691 8692 8693 8694 8695 8696 8697 8698 8699 8700 8701 8702 8703 8704 8705 8706 8707 8708 8709 8710 8711 8712 8713 8714 8715 8716 8717 8718 8719 8720 8721 8722 8723 8724 8725 8726 8727 8728 8729 8730 8731 8732 8733 8734 8735 8736 8737 8738 8739 8740 8741 8742 8743 8744 8745 8746 8747 8748 8749 8750 8751 8752 8753 8754 8755 8756 8757 8758 8759 8760 8761 8762 8763 8764 8765 8766 8767 8768 8769 8770 8771 8772 8773 8774 8775 8776 8777 8778 8779 8780 8781 8782 8783 8784 8785 8786 8787 8788 8789 8790 8791 8792 8793 8794 8795 8796 8797 8798 8799 8800 8801 8802 8803 8804 8805 8806 8807 8808 8809 8810 8811 8812 8813 8814 8815 8816 8817 8818 8819 8820 8821 8822 8823 8824 8825 8826 8827 8828 8829 8830 8831 8832 8833 8834 8835 8836 8837 8838 8839 8840 8841 8842 8843 8844 8845 8846 8847 8848 8849 8850 8851 8852 8853 8854 8855 8856 8857 8858 8859 8860 8861 8862 8863 8864
|
#
# This file is the units database for use with GNU units, a units conversion
# program by Adrian Mariano adrianm@gnu.org
#
# Version 3.22
# last updated 22 November 2024
#
# Copyright (C) 1996-2002, 2004-2020, 2022, 2024
# Free Software Foundation, Inc
#
# This program is free software; you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation; either version 3 of the License, or
# (at your option) any later version.
#
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU General Public License
# along with this program; if not, write to the Free Software
# Foundation, Inc., 51 Franklin Street, Fifth Floor,
# Boston, MA 02110-1301 USA
#
############################################################################
#
# Improvements and corrections are welcome.
#
# See the end of this file for a list of items we have chosen to exclude
# or have decided are out of scope for GNU units.
#
# Fundamental constants in this file are the 2018 CODATA recommended values.
#
# Most units data was drawn from
# 1. NIST Special Publication 811, Guide for the
# Use of the International System of Units (SI).
# Barry N. Taylor. 2008
# https://www.nist.gov/pml/special-publication-811
# 2. CRC Handbook of Chemistry and Physics 70th edition
# 3. Oxford English Dictionary
# 4. Webster's New Universal Unabridged Dictionary
# 5. Units of Measure by Stephen Dresner
# 6. A Dictionary of English Weights and Measures by Ronald Zupko
# 7. British Weights and Measures by Ronald Zupko
# 8. Realm of Measure by Isaac Asimov
# 9. United States standards of weights and measures, their
# creation and creators by Arthur H. Frazier.
# 10. French weights and measures before the Revolution: a
# dictionary of provincial and local units by Ronald Zupko
# 11. Weights and Measures: their ancient origins and their
# development in Great Britain up to AD 1855 by FG Skinner
# 12. The World of Measurements by H. Arthur Klein
# 13. For Good Measure by William Johnstone
# 14. NTC's Encyclopedia of International Weights and Measures
# by William Johnstone
# 15. Sizes by John Lord
# 16. Sizesaurus by Stephen Strauss
# 17. CODATA Recommended Values of Physical Constants available at
# http://physics.nist.gov/cuu/Constants/index.html
# 18. How Many? A Dictionary of Units of Measurement. Available at
# http://www.ibiblio.org/units/
# 19. Numericana. http://www.numericana.com
# 20. UK history of measurement
# https://metrication.uk/more/timeline/
# 21. NIST Handbook 44, Specifications, Tolerances, and
# Other Technical Requirements for Weighing and Measuring
# Devices. 2011
# 22. NIST Special Publication 447, Weights and Measures Standards
# of the United States: a brief history. Lewis V. Judson.
# 1963; rev. 1976
# 23. CRC Handbook of Chemistry and Physics, 96th edition
# 24. Dictionary of Scientific Units, 6th ed. H.G. Jerrard and D.B.
# McNeill. 1992
# 25. NIST Special Publication 330, The International System of
# Units (SI). ed. Barry N. Taylor and Ambler Thompson. 2008
# https://www.nist.gov/pml/special-publication-330
# 26. BIPM Brochure, The International System of Units (SI).
# 9th ed., 2019
# https://www.bipm.org/en/publications/si-brochure/
#
###########################################################################
#
# If units you use are missing or defined incorrectly, please contact me.
# If your country's local units are missing and you are willing to supply
# them, please send me a list.
#
###########################################################################
###########################################################################
#
# Brief Philosophy of this file
#
# Most unit definitions are made in terms of integers or simple fractions of
# other definitions. The typical exceptions are when converting between two
# different unit systems, or the values of measured physical constants. In
# this file definitions are given in the most natural and revealing way in
# terms of integer factors.
#
# If you make changes be sure to run 'units --check' to check your work.
#
# The file is USA-centric, but there is some modest effort to support other
# countries. This file is now coded in UTF-8. To support environments where
# UTF-8 is not available, definitions that require this character set are
# wrapped in !utf8 directives.
#
# When a unit name is used in different countries with the different meanings
# the system should be as follows:
#
# Suppose countries ABC and XYZ both use the "foo". Then globally define
#
# ABCfoo <some value>
# XYZfoo <different value>
#
# Then, using the !locale directive, define the "foo" appropriately for each of
# the two countries with a definition like
#
# !locale ABC
# foo ABCfoo
# !endlocale
#
###########################################################################
!locale en_US
! set UNITS_ENGLISH US
!endlocale
!locale en_GB
! set UNITS_ENGLISH GB
!endlocale
!set UNITS_ENGLISH US # Default setting for English units
!set UNITS_SYSTEM default # Set a default value
!varnot UNITS_SYSTEM si emu esu gaussian gauss hlu natural natural-gauss hartree planck planck-red default
!message Unknown unit system given with -u or UNITS_SYSTEM environment variable
!message Valid systems: si, emu, esu, gauss[ian], hlu, natural, natural-gauss
!message planck, planck-red, hartree
!message Using SI
!prompt (SI)
!endvar
!var UNITS_SYSTEM si
!message SI units selected
!prompt (SI)
!endvar
###########################################################################
# #
# Primitive units. Any unit defined to contain a '!' character is a #
# primitive unit which will not be reduced any further. All units should #
# reduce to primitive units. #
# #
###########################################################################
#
# SI units
#
# On 20 May 2019, the SI was revised to define the units by fixing the
# values of physical constants that depend on those units.
#
# https://www.nist.gov/si-redefinition/
#
# The BIPM--the International Bureau of Weights and Measures--provides a
# succinct description of the new SI in its Concise Summary:
#
# https://www.bipm.org/utils/common/pdf/si-brochure/SI-Brochure-9-concise-EN.pdf
#
# The SI is the system of units in which:
#
# * the unperturbed ground state hyperfine transition frequency of the
# caesium 133 atom is delta nu_Cs = 9 192 631 770 Hz,
# * the speed of light in vacuum, c, is 299 792 458 m/s,
# * the Planck constant, h, is 6.626 070 15 * 10^-34 J s,
# * the elementary charge, e, is 1.602 176 634 * 10^-19 C,
# * the Boltzmann constant, k, is 1.380 649 * 10^-23 J/K,
# * the Avogadro constant, N_A, is 6.022 140 76 * 10^23 mol^-1,
# * the luminous efficacy of monochromatic radiation of frequency
# 540 * 10^12 Hz, K_cd, is 683 lm/W,
#
# where the hertz, joule, coulomb, lumen, and watt, with unit symbols Hz,
# J, C, lm, and W, respectively, are related to the units second, metre,
# kilogram, ampere, kelvin, mole, and candela, with unit symbols s, m, kg,
# A, K, mol, and cd, respectively, according to Hz = s^-1, J = kg m^2 s^-2,
# C = A s, lm = cd m^2 m^-2 = cd sr, and W = kg m^2 s^-3.
#
# These definitions specify the exact numerical value of each constant when
# its value is expressed in the corresponding SI unit. By fixing the exact
# numerical value the unit becomes defined, since the product of the
# numerical value and the unit has to equal the value of the constant,
# which is invariant.
#
# The defining constants have been chosen such that, when taken together,
# their units cover all of the units of the SI. In general, there is no
# one-to-one correspondence between the defining constants and the SI base
# units. Any SI unit is a product of powers of these seven constants and a
# dimensionless factor.
#
# Until 2018, the SI was defined in terms of base units and derived units.
# These categories are no longer essential in the SI, but they are maintained
# in view of their convenience and widespread use. They are arguably more
# intuitive than the new definitions. (They are also essential to the
# operation of GNU units.) The definitions of the base units, which follow
# from the definition of the SI in terms of the seven defining constants, are
# given below.
#
s ! # The second, symbol s, is the SI unit of time. It is defined
second s # by taking the fixed numerical value of the unperturbed
# ground-state hyperfine transition frequency of the
# cesium-133 atom to be 9 192 631 770 when expressed in the
# unit Hz, which is equal to 1/s.
#
# This definition is a restatement of the previous one, the
# duration of 9192631770 periods of the radiation corresponding
# to the cesium-133 transition.
nu_133Cs 9192631770 Hz # Cesium-133 transition frequency (exact)
c_SI 299792458
c 299792458 m/s # speed of light in vacuum (exact)
m ! # The metre, symbol m, is the SI unit of length. It is
meter m # defined by taking the fixed numerical value of the speed
metre m # of light in vacuum, c, to be 299 792 458 when expressed in
# units of m/s.
#
# This definition is a rewording of the previous one and is
# equivalent to defining the meter as the distance light
# travels in 1|299792458 seconds. The meter was originally
# intended to be 1e-7 of the length along a meridian from the
# equator to a pole.
h_SI 6.62607015e-34
h 6.62607015e-34 J s # Planck constant (exact)
kg ! # The kilogram, symbol kg, is the SI unit of mass. It is
kilogram kg # defined by taking the fixed numerical value of the Planck
# constant, h, to be 6.626 070 15 * 10^-34 when expressed in
# the unit J s which is equal to kg m^2 / s.
#
# One advantage of fixing h to define the kilogram is that this
# affects constants used to define the ampere. If the kg were
# defined by directly fixing the mass of something, then h
# would be subject to error.
#
# The previous definition of the kilogram was the mass of the
# international prototype kilogram. The kilogram was the last
# unit whose definition relied on reference to an artifact.
#
# It is not obvious what this new definition means, or
# intuitively how fixing Planck's constant defines the
# kilogram. To define the kilogram we need to give the mass
# of some reference in kilograms. Previously the prototype in
# France served as this reference, and it weighed exactly 1
# kg. But the reference can have any weight as long as you
# know the weight of the reference. The new definition uses
# the "mass" of a photon, or more accurately, the mass
# equivalent of the energy of a photon. The energy of a
# photon depends on its frequency. If you pick a frequency,
# f, then the energy of the photon is hf, and hence the mass
# equivalent is hf/c^2. If we reduce this expression using
# the constant defined values for h and c the result is a
# value in kilograms for the mass-equivalent of a photon of
# frequency f, which can therefore define the size of the
# kilogram.
#
# For more on the relationship between mass an Planck's
# constant:
#
# https://www.nist.gov/si-redefinition/kilogram-mass-and-plancks-constant
# This definition may still seem rather abstract: you can't
# place a "kilogram of radiation" on one side of a balance.
# Metrologists realize the kilogram using a Kibble Balance, a
# device which relates mechanical energy to electrical energy
# and can measure mass with extreme accuracy if h is known.
#
# For more on the Kibble Balance see
#
# https://www.nist.gov/si-redefinition/kilogram-kibble-balance
# https://en.wikipedia.org/wiki/Kibble_balance
k_SI 1.380649e-23
boltzmann 1.380649e-23 J/K # Boltzmann constant (exact)
k boltzmann
K ! # The kelvin, symbol K, is the SI unit of thermodynamic
kelvin K # temperature. It is defined by taking the fixed numerical
# value of the Boltzmann constant, k, to be 1.380 649 * 10^-23
# when expressed in the unit J/K, which is equal to
# kg m^2/s^2 K.
#
# The boltzmann constant establishes the relationship between
# energy and temperature. The average thermal energy carried
# by each degree of freedom is kT/2. A monatomic ideal gas
# has three degrees of freedom corresponding to the three
# spatial directions, which means its thermal energy is
# (3/2) k T.
#
# The previous definition of the kelvin was based on the
# triple point of water. The change in the definition of the
# kelvin will not have much effect on measurement practice.
# Practical temperature calibration makes use of two scales,
# the International Temperature Scale of 1990 (ITS-90), which
# covers the range of 0.65 K to 1357.77K and the Provisional
# Low Temperature Scale of 2000 (PLTS-2000), which covers the
# range of 0.9 mK to 1 K.
# https://www.bipm.org/en/committees/cc/cct/publications-cc.html
#
# The ITS-90 contains 17 reference points including things
# like the triple point of hydrogen (13.8033 K) or the
# freezing point of gold (1337.33 K), and of course the triple
# point of water. The PLTS-2000 specifies four reference
# points, all based on properties of helium-3.
#
# The redefinition of the kelvin will not affect the values of
# these reference points, which have been determined by
# primary thermometry, using thermometers that rely only on
# relationships that allow temperature to be calculated
# directly without using any unknown quantities. Examples
# include acoustic thermometers, which measure the speed of
# sound in a gas, or electronic thermometers, which measure
# tiny voltage fluctuations in resistors. Both variables
# depend directly on temperature.
e_SI 1.602176634e-19
e 1.602176634e-19 C # electron charge (exact)
A ! # The ampere, symbol A, is the SI unit of electric current.
ampere A # It is defined by taking the fixed numerical value of the
amp ampere # elementary charge, e, to be 1.602 176 634 * 10^-19 when
# expressed in the unit C, which is equal to A*s.
#
# The previous definition was the current which produces a
# force of 2e-7 N/m between two infinitely long wires a meter
# apart. This definition was difficult to realize accurately.
#
# The ampere is actually realized by establishing the volt and
# the ohm, since A = V / ohm. These measurements can be done
# using the Josephson effect and the quantum Hall effect,
# which accurately measure voltage and resistance, respectively,
# with reference to two fixed constants, the Josephson
# constant, K_J=2e/h and the von Klitzing constant, R_K=h/e^2.
# Under the previous SI system, these constants had official
# fixed values, defined in 1990. This created a situation
# where the standard values for the volt and ohm were in some
# sense outside of SI because they depended primarily on
# constants different from the ones used to define SI. After
# the revision, since e and h have exact definitions, the
# Josephson and von Klitzing constants will also have exact
# definitions that derive from SI instead of the conventional
# 1990 values.
#
# In fact we know that there is a small offset between the
# conventional values of the electrical units based on the
# conventional 1990 values and the SI values. The new
# definition, which brings the practical electrical units back
# into SI, will lead to a one time change of +0.1ppm for
# voltage values and +0.02ppm for resistance values.
#
# The previous definition resulted in fixed exact values for
# the vacuum permeability (mu0), the impedance of free space
# (Z0), the vacuum permittivity (epsilon0), and the Coulomb
# constant. With the new definition, these four values are
# subject to experimental error.
avogadro 6.02214076e23 / mol # Size of a mole (exact)
N_A avogadro
mol ! # The mole, symbol mol, is the SI unit of amount of
mole mol # substance. One mole contains exactly 6.022 140 76 * 10^23
# elementary entities. This number is the fixed numerical
# value of the Avogadro constant, N_A, when expressed in the
# unit 1/mol and is called the Avogadro number. The amount of
# substance, symbol n, of a system is a measure of the number
# of specified elementary entities. An elementary entity may
# be an atom, a molecule, an ion, an electron, any other
# particle or specified group of particles.
#
# The atomic mass unit (u) is defined as 1/12 the mass of
# carbon-12. Previously the mole was defined so that a mole
# of carbon-12 weighed exactly 12g, or N_A u = 1 g/mol
# exactly. This relationship is now an experimental,
# approximate relationship.
#
# To determine the size of the mole, researchers used spheres
# of very pure silicon-28 that weighed a kilogram. They
# measured the molar mass of Si-28 using mass spectrometry and
# used X-ray diffraction interferometry to determine the
# spacing of the silicon atoms in the sphere. Using the
# sphere's volume it was then possible to determine the number
# of silicon atoms in the sphere, and hence determine the
# Avogadro constant. The results of this experiment were used
# to define N_A, which is henceforth a fixed, unchanging
# quantity.
cd ! # The candela, symbol cd, is the SI unit of luminous intensity
candela cd # in a given direction. It is defined by taking the fixed
# numerical value of the luminous efficacy of monochromatic
# radiation of the frequency 540e12 Hz to be 683 when
# expressed in the unit lumen/watt, which is equal to
# cd sr/W, or cd sr s^3/kg m^2
#
# This definition is a rewording of the previous definition.
# Luminous intensity differs from radiant intensity (W/sr) in
# that it is adjusted for human perceptual dependence on
# wavelength. The frequency of 540e12 Hz (yellow;
# wavelength approximately 555 nm in vacuum) is where human
# perception is most efficient.
K_cd 683 lumen/W # Luminous efficiency at 540e12 Hz (exact)
# Angular Measure
#
# The radian and steradian are defined as dimensionless primitive units.
# The radian is equal to m/m and the steradian to m^2/m^2 so these units are
# dimensionless. Retaining them as named units is useful because it allows
# clarity in expressions and makes the meaning of unit definitions more clear.
# These units will reduce to 1 in conversions but not for sums of units or for
# arguments to functions.
#
radian !dimensionless # Plane angle subtended at the center of a circle by
# an arc equal in length to the radius of the
# circle.
# Dimension: LENGTH (of arc) / DISTANCE (radius)
sr !dimensionless # Solid angle which cuts off an area of the surface
steradian sr # of the sphere equal to that of a square with
# sides of length equal to the radius of the
# sphere.
# Dimension: AREA (of surface) / DISTANCE^2
# (radius^2)
#
# A primitive non-SI unit
#
bit ! # Basic unit of information (entropy). The entropy in bits
# of a random variable over a finite alphabet is defined
# to be the sum of -p(i)*log2(p(i)) over the alphabet where
# p(i) is the probability that the random variable takes
# on the value i.
#
# Currency: the primitive unit of currency is defined in currency.units.
# It is usually the US$ or the euro, but it is user selectable.
#
#
# Absolute value
#
abs(x) noerror sqrt(x^2)
###########################################################################
# #
# Prefixes (longer names must come first) #
# #
###########################################################################
quetta- 1e30 # Allegedly from "q" plus Greek "deka" (ten)
ronna- 1e27 # Allegedly from "r" plus Greek "ennea" (nine)
yotta- 1e24 # Greek or Latin "octo" (eight)
zetta- 1e21 # Latin "septem" (seven)
exa- 1e18 # Greek "hex" (six)
peta- 1e15 # Greek "pente" (five)
tera- 1e12 # Greek "teras" (monster)
giga- 1e9 # Greek "gigas" (giant)
mega- 1e6 # Greek "megas" (large)
myria- 1e4 # Not an official SI prefix
kilo- 1e3 # Greek "chilioi" (thousand)
hecto- 1e2 # Greek "hekaton" (hundred)
deca- 1e1 # Greek "deka" (ten)
deka- deca
deci- 1e-1 # Latin "decimus" (tenth)
centi- 1e-2 # Latin "centum" (hundred)
milli- 1e-3 # Latin "mille" (thousand)
micro- 1e-6 # Latin "micro" or Greek "mikros" (small)
nano- 1e-9 # Latin "nanus" or Greek "nanos" (dwarf)
pico- 1e-12 # Spanish "pico" (a bit)
femto- 1e-15 # Danish-Norwegian "femten" (fifteen)
atto- 1e-18 # Danish-Norwegian "atten" (eighteen)
zepto- 1e-21 # Latin "septem" (seven)
yocto- 1e-24 # Greek or Latin "octo" (eight)
ronto- 1e-27 # Allegedly "r" plus Latin "novum" (nine)
quecto- 1e-30 # Allegedly "q" plus Latin "decim" (ten)
quarter- 1|4
semi- 0.5
demi- 0.5
hemi- 0.5
half- 0.5
double- 2
triple- 3
treble- 3
kibi- 2^10 # In response to the improper and confusing
mebi- 2^20 # use of SI prefixes for powers of two,
gibi- 2^30 # the International Electrotechnical
tebi- 2^40 # Commission aproved these binary prefixes
pebi- 2^50 # in IEC 60027-2 Amendment 2 (1999).
exbi- 2^60
zebi- 2^70 # Zebi- and yobi- were added in the 2005 ed.,
yobi- 2^80 # later superseded by ISO/IEC 80000-13:2008.
robi- 2^90
quebi- 2^100
Ki- kibi
Mi- mebi
Gi- gibi
Ti- tebi
Pi- pebi
Ei- exbi
Zi- zebi
Yi- yobi
Ri- robi
Qi- quebi
Q- quetta
R- ronna
Y- yotta
Z- zetta
E- exa
P- peta
T- tera
G- giga
M- mega
k- kilo
h- hecto
da- deka
d- deci
c- centi
m- milli
u- micro # it should be a mu but u is easy to type
n- nano
p- pico
f- femto
a- atto
z- zepto
y- yocto
r- ronto
q- quecto
#
# Names of some numbers
#
one 1
two 2
double 2
couple 2
three 3
triple 3
four 4
quadruple 4
five 5
quintuple 5
six 6
seven 7
eight 8
nine 9
ten 10
eleven 11
twelve 12
thirteen 13
fourteen 14
fifteen 15
sixteen 16
seventeen 17
eighteen 18
nineteen 19
twenty 20
thirty 30
forty 40
fifty 50
sixty 60
seventy 70
eighty 80
ninety 90
hundred 100
thousand 1000
million 1e6
twoscore two score
threescore three score
fourscore four score
fivescore five score
sixscore six score
sevenscore seven score
eightscore eight score
ninescore nine score
tenscore ten score
twelvescore twelve score
# These number terms were described by N. Chuquet and De la Roche in the 16th
# century as being successive powers of a million. These definitions are still
# used in most European countries. The current US definitions for these
# numbers arose in the 17th century and don't make nearly as much sense. These
# numbers are listed in the CRC Concise Encyclopedia of Mathematics by Eric
# W. Weisstein.
shortbillion 1e9
shorttrillion 1e12
shortquadrillion 1e15
shortquintillion 1e18
shortsextillion 1e21
shortseptillion 1e24
shortoctillion 1e27
shortnonillion 1e30
shortnoventillion shortnonillion
shortdecillion 1e33
shortundecillion 1e36
shortduodecillion 1e39
shorttredecillion 1e42
shortquattuordecillion 1e45
shortquindecillion 1e48
shortsexdecillion 1e51
shortseptendecillion 1e54
shortoctodecillion 1e57
shortnovemdecillion 1e60
shortvigintillion 1e63
centillion 1e303
googol 1e100
longbillion million^2
longtrillion million^3
longquadrillion million^4
longquintillion million^5
longsextillion million^6
longseptillion million^7
longoctillion million^8
longnonillion million^9
longnoventillion longnonillion
longdecillion million^10
longundecillion million^11
longduodecillion million^12
longtredecillion million^13
longquattuordecillion million^14
longquindecillion million^15
longsexdecillion million^16
longseptdecillion million^17
longoctodecillion million^18
longnovemdecillion million^19
longvigintillion million^20
# These numbers fill the gaps left by the long system above.
milliard 1000 million
billiard 1000 million^2
trilliard 1000 million^3
quadrilliard 1000 million^4
quintilliard 1000 million^5
sextilliard 1000 million^6
septilliard 1000 million^7
octilliard 1000 million^8
nonilliard 1000 million^9
noventilliard nonilliard
decilliard 1000 million^10
# For consistency
longmilliard milliard
longbilliard billiard
longtrilliard trilliard
longquadrilliard quadrilliard
longquintilliard quintilliard
longsextilliard sextilliard
longseptilliard septilliard
longoctilliard octilliard
longnonilliard nonilliard
longnoventilliard noventilliard
longdecilliard decilliard
# The long centillion would be 1e600. The googolplex is another
# familiar large number equal to 10^googol. These numbers give overflows.
#
# The short system prevails in English speaking countries
#
billion shortbillion
trillion shorttrillion
quadrillion shortquadrillion
quintillion shortquintillion
sextillion shortsextillion
septillion shortseptillion
octillion shortoctillion
nonillion shortnonillion
noventillion shortnoventillion
decillion shortdecillion
undecillion shortundecillion
duodecillion shortduodecillion
tredecillion shorttredecillion
quattuordecillion shortquattuordecillion
quindecillion shortquindecillion
sexdecillion shortsexdecillion
septendecillion shortseptendecillion
octodecillion shortoctodecillion
novemdecillion shortnovemdecillion
vigintillion shortvigintillion
#
# Numbers used in India
#
lakh 1e5
crore 1e7
arab 1e9
kharab 1e11
neel 1e13
padm 1e15
shankh 1e17
#############################################################################
# #
# Derived units which can be reduced to the primitive units #
# #
#############################################################################
#
# Named SI derived units (officially accepted)
#
newton kg m / s^2 # force
N newton
pascal N/m^2 # pressure or stress
Pa pascal
joule N m # energy
J joule
watt J/s # power
W watt
coulomb A s # charge
C coulomb
volt W/A # potential difference
V volt
ohm V/A # electrical resistance
siemens A/V # electrical conductance
S siemens
farad C/V # capacitance
F farad
weber V s # magnetic flux
Wb weber
henry V s / A # inductance, also Wb/A, but needs to be
H henry # defined this way for CGS units
tesla Wb/m^2 # magnetic flux density
T tesla
hertz /s # frequency
Hz hertz
#
# Dimensions. These are here to help with dimensional analysis and
# because they will appear in the list produced by hitting '?' at the
# "You want:" prompt to tell the user the dimension of the unit.
#
LENGTH meter
AREA LENGTH^2
VOLUME LENGTH^3
MASS kilogram
AMOUNT mole
ANGLE radian
SOLID_ANGLE steradian
MONEY US$
FORCE newton
TORQUE FORCE DISTANCE
PRESSURE FORCE / AREA
STRESS FORCE / AREA
FREQUENCY hertz
WAVELENGTH LENGTH
WAVENUMBER 1/WAVELENGTH # number of waves per distance
VELOCITY DISPLACEMENT / TIME # a vector (includes direction)
SPEED DISTANCE / TIME # a scalar
ACCELERATION VELOCITY / TIME
MOMENTUM MASS VELOCITY # Also ENERGY / VELOCITY or IMPULSE
IMPULSE FORCE TIME
DISPLACEMENT LENGTH
DISTANCE LENGTH
ELONGATION LENGTH
STRAIN ELONGATION / LENGTH
ENERGY joule
POWER watt
WORK FORCE DISTANCE
DENSITY MASS / VOLUME
LINEAR_DENSITY MASS / LENGTH
SPECIFIC_ENERGY ENERGY / MASS
VISCOSITY FORCE TIME / AREA
KINEMATIC_VISCOSITY VISCOSITY / DENSITY
CURRENT ampere
CHARGE coulomb
CAPACITANCE farad
RESISTANCE ohm
CONDUCTANCE siemens
# It may be easier to understand the relationship by considering
# an object with specified dimensions and resistivity, whose
# resistance is given by the resistivity * length / area.
RESISTIVITY RESISTANCE AREA / LENGTH
CONDUCTIVITY CONDUCTANCE LENGTH / AREA
INDUCTANCE henry
E_FIELD ELECTRIC_POTENTIAL / LENGTH
B_FIELD tesla
# The D and H fields are related to the E and B fields by factors of
# epsilon (electric permittivity) and mu (magnetic permeability)
# respectively. The definitions of permittivity and permeability
# below are scaled to make it possible to convert D_FIELD and
# E_FIELD between SI and CGS units.
ELECTRIC_PERMITTIVITY epsilon0 / epsilon0_SI # SI: F/m
MAGNETIC_PERMEABILITY mu0 / mu0_SI # SI: H/m = N/A^2
D_FIELD E_FIELD ELECTRIC_PERMITTIVITY
H_FIELD B_FIELD / MAGNETIC_PERMEABILITY
ELECTRIC_DIPOLE_MOMENT CHARGE DISTANCE
MAGNETIC_DIPOLE_MOMENT TORQUE / B_FIELD
POLARIZATION ELECTRIC_DIPOLE_MOMENT / VOLUME
MAGNETIZATION MAGNETIC_DIPOLE_MOMENT / VOLUME
ELECTRIC_POTENTIAL ENERGY / CHARGE # volt
VOLTAGE ELECTRIC_POTENTIAL
E_FLUX E_FIELD AREA
D_FLUX D_FIELD AREA
B_FLUX B_FIELD AREA
H_FLUX H_FIELD AREA
#
# units derived easily from SI units
#
gram millikg
gm gram
g gram
tonne 1000 kg
t tonne
metricton tonne
sthene tonne m / s^2
funal sthene
pieze sthene / m^2
quintal 100 kg
bar 1e5 Pa # About 1 atm
b bar
vac millibar
micron micrometer # One millionth of a meter
bicron picometer # One brbillionth of a meter
cc cm^3
liter 1000 cc # The liter was defined in 1901 as the
oldliter 1.000028 dm^3 # space occupied by 1 kg of pure water at
L liter # the temperature of its maximum density
l liter # under a pressure of 1 atm. This was
# supposed to be 1000 cubic cm, but it
# was discovered that the original
# measurement was off. In 1964, the
# liter was redefined to be exactly 1000
# cubic centimeters.
Ah amp hour # Unit of charge
mho siemens # Inverse of ohm, hence ohm spelled backward
galvat ampere # Named after Luigi Galvani
angstrom 1e-10 m # Convenient for describing molecular sizes
xunit xunit_cu # Used for measuring x-ray wavelengths.
siegbahn xunit # Originally defined to be 1|3029.45 of
xunit_cu 1.00207697e-13 m # the spacing of calcite planes at 18
xunit_mo 1.00209952e-13 m # degC. It was intended to be exactly
# 1e-13 m, but was later found to be
# slightly off. Current usage is with
# reference to common x-ray lines, either
# the K-alpha 1 line of copper or the
# same line of molybdenum.
angstromstar 1.00001495 angstrom # Defined by JA Bearden in 1965 to replace
# the X unit. The wavelength of the
# tungsten K alpha1 line was defined as
# exactly 0.20901 angstrom star, with the
# value chosen to try to make the new
# unit close to the angstrom.
silicon_d220 1.920155716e-10 m # Silicon lattice spacing
siliconlattice sqrt(8) silicon_d220# Silicon lattice parameter, (a), the side
# length of the unit cell for the diamond
# centered cubic structure of silicon.
fermi 1e-15 m # Convenient for describing nuclear sizes
# Nuclear radius is from 1 to 10 fermis
barn 1e-28 m^2 # Used to measure cross section for
# particle physics collision, said to
# have originated in the phrase "big as
# a barn".
shed 1e-24 barn # Defined to be a smaller companion to the
# barn, but it's too small to be of
# much use.
brewster micron^2/N # measures stress-optical coef
diopter /m # measures reciprocal of lens focal length
fresnel 1e12 Hz # occasionally used in spectroscopy
shake 1e-8 sec
svedberg 1e-13 s # Used for measuring the sedimentation
# coefficient for centrifuging.
gamma microgram # Also used for 1e-9 tesla
lambda microliter
spat 1e12 m # Rarely used for astronomical measurements
preece 1e13 ohm m # resistivity
planck J s # action of one joule over one second
sturgeon /henry # magnetic reluctance
daraf 1/farad # elastance (farad spelled backwards)
leo 10 m/s^2
poiseuille N s / m^2 # viscosity
mayer J/g K # specific heat
mired / microK # reciprocal color temperature. The name
# abbreviates micro reciprocal degree.
crocodile megavolt # used informally in UK physics labs
metricounce 25 g
mounce metricounce
finsenunit 1e5 W/m^2 # Measures intensity of ultraviolet light
# with wavelength 296.7 nm.
fluxunit 1e-26 W/m^2 Hz # Used in radio astronomy to measure
# the energy incident on the receiving
# body across a specified frequency
# bandwidth. [12]
jansky fluxunit # K. G. Jansky identified radio waves coming
Jy jansky # from outer space in 1931.
flick W / cm^2 sr micrometer # Spectral radiance or irradiance
pfu / cm^2 sr s # particle flux unit -- Used to measure
# rate at which particles are received by
# a spacecraft as particles per solid
# angle per detector area per second. [18]
pyron cal_IT / cm^2 min # Measures heat flow from solar radiation,
# from Greek work "pyr" for fire.
katal mol/sec # Measure of the amount of a catalyst. One
kat katal # katal of catalyst enables the reaction
# to consume or produce one mol/sec.
solarluminosity 382.8e24 W # A common yardstick for comparing the
# output of different stars.
# http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html
# at mean Earth-Sun distance
solarirradiance solarluminosity / (4 pi sundist^2)
solarconstant solarirradiance
TSI solarirradiance # total solar irradiance
#
# Land Area
#
# The are was defined by an earlier form of SI. Many countries
# redefined old land area units to equal the decare (10 are)
#
are 100 m^2
a are
sotka are # Russian
stremma decare # Greece
dunam decare # Different spellings of the old
dulum decare # Ottoman measure
donum decare #
!utf8
dönüm decare
mål decare # Norway.
!endutf8
#
# time
#
sec s
minute 60 s
min minute
hour 60 min
hr hour
day 24 hr
d day
da day
week 7 day
wk week
sennight 7 day
fortnight 14 day
blink 1e-5 day # Actual human blink takes 1|3 second
ce 1e-2 day
cron 1e6 years
watch 4 hours # time a sentry stands watch or a ship's
# crew is on duty.
bell 1|8 watch # Bell would be sounded every 30 minutes.
# French Revolutionary Time or Decimal Time. It was Proposed during
# the French Revolution. A few clocks were made, but it never caught
# on. In 1998 Swatch defined a time measurement called ".beat" and
# sold some watches that displayed time in this unit.
decimalhour 1|10 day
decimalminute 1|100 decimalhour
decimalsecond 1|100 decimalminute
beat decimalminute # Swatch Internet Time
#
# angular measure
#
circle 2 pi radian
degree 1|360 circle
deg degree
arcdeg degree
arcmin 1|60 degree
arcminute arcmin
' arcmin
arcsec 1|60 arcmin
arcsecond arcsec
" arcsec
'' "
!utf8
° degree
′ ' # prime, U+2032
″ " # double prime, U+2033
!endutf8
rightangle 90 degrees
quadrant 1|4 circle
quintant 1|5 circle
sextant 1|6 circle
sign 1|12 circle # Angular extent of one sign of the zodiac
turn circle
revolution turn
rev turn
pulsatance radian / sec
gon 1|100 rightangle # measure of grade
grade gon
centesimalminute 1|100 grade
centesimalsecond 1|100 centesimalminute
milangle 1|6400 circle # Official NIST definition.
# Another choice is 1e-3 radian.
pointangle 1|32 circle # Used for reporting compass readings
centrad 0.01 radian # Used for angular deviation of light
# through a prism.
mas milli arcsec # Used by astronomers
seclongitude circle (seconds/day) # Astronomers measure longitude
# (which they call right ascension) in
# time units by dividing the equator into
# 24 hours instead of 360 degrees.
#
# Some geometric formulas
#
circum(r) units=[m;m] range=[0,) 2 pi r; circum/ 2 pi
circum_d(d) units=[m;m] range=[0,) circum(d/2); 2 ~circum(circum_d)
circlearea(r) units=[m;m^2] range=[0,) pi r^2 ; sqrt(circlearea/pi)
circlearea_d(d) units=[m;m^2] range=[0,) circlearea(d/2); 2 ~circlearea(circlearea_d)
spherevolume(r) units=[m;m^3] range=[0,) 4|3 pi r^3 ; \
cuberoot(spherevolume/4|3 pi)
spherevolume_d(d) units=[m;m^3] range=[0,) spherevolume(d/2); 2 ~spherevolume(spherevolume_d)
spherevol() spherevolume
spherevol_d() spherevolume_d
circumference() circum
circumference_d() circum_d
square(x) range=[0,) x^2 ; sqrt(square)
cube(x) range=[0,) x^3 ; cube^(1|3)
#
# Solid angle measure
#
sphere 4 pi sr
squaredegree 1|180^2 pi^2 sr
squareminute 1|60^2 squaredegree
squaresecond 1|60^2 squareminute
squarearcmin squareminute
squarearcsec squaresecond
sphericalrightangle 1|8 sphere
octant 1|8 sphere
#
# Concentration measures
#
percent 0.01
% percent
mill 0.001 # Originally established by Congress in 1791
# as a unit of money equal to 0.001 dollars,
# it has come to refer to 0.001 in general.
# Used by some towns to set their property
# tax rate, and written with a symbol similar
# to the % symbol but with two 0's in the
# denominator. [18]
proof 1|200 # Alcohol content measured by volume at
# 60 degrees Fahrenheit. This is a USA
# measure. In Europe proof=percent.
ppm 1e-6
partspermillion ppm
ppb 1e-9
partsperbillion ppb # USA billion
ppt 1e-12
partspertrillion ppt # USA trillion
karat 1|24 # measure of gold purity
caratgold karat
gammil mg/l
basispoint 0.01 % # Used in finance
fine 1|1000 # Measure of gold purity
# The pH scale is used to measure the concentration of hydronium (H3O+) ions in
# a solution. A neutral solution has a pH of 7 as a result of dissociated
# water molecules.
pH(x) units=[1;mol/liter] range=(0,) 10^(-x) mol/liter ; (-log(pH liters/mol))
#
# Temperature
#
# Two types of units are defined: units for converting temperature differences
# and functions for converting absolute temperatures. Conversions for
# differences start with "deg" and conversions for absolute temperature start
# with "temp".
#
# If the temperature inside is 72 degrees Fahrenheit and you want to
# convert this to degrees Celsius then you need absolute temperature:
#
# You have: tempF(72)
# You want: tempC
# 22.222222
#
# If the temperature rose 72 degrees Fahrenheit during the chemical reaction
# then this is a temperature difference:
#
# You have: 72 degF
# You want: degC
# * 40
# / 0.025
#
TEMPERATURE kelvin
TEMPERATURE_DIFFERENCE kelvin
# In 1741 Anders Celsius introduced a temperature scale with water boiling at
# 0 degrees and freezing at 100 degrees at standard pressure. After his death
# the fixed points were reversed and the scale was called the centigrade
# scale. Due to the difficulty of accurately measuring the temperature of
# melting ice at standard pressure, the centigrade scale was replaced in 1954
# by the Celsius scale which is defined by subtracting 273.15 from the
# temperature in Kelvins. This definition differed slightly from the old
# centigrade definition, but the Kelvin scale depends on the triple point of
# water rather than a melting point, so it can be measured accurately.
tempC(x) units=[1;K] domain=[-273.15,) range=[0,) \
x K + stdtemp ; (tempC +(-stdtemp))/K
tempcelsius() tempC
degcelsius K
degC K
# Fahrenheit defined his temperature scale by setting 0 to the coldest
# temperature he could produce in his lab with a salt water solution and by
# setting 96 degrees to body heat. In Fahrenheit's words:
#
# Placing the thermometer in a mixture of sal ammoniac or sea
# salt, ice, and water a point on the scale will be found which
# is denoted as zero. A second point is obtained if the same
# mixture is used without salt. Denote this position as 30. A
# third point, designated as 96, is obtained if the thermometer
# is placed in the mouth so as to acquire the heat of a healthy
# man." (D. G. Fahrenheit, Phil. Trans. (London) 33, 78, 1724)
tempF(x) units=[1;K] domain=[-459.67,) range=[0,) \
(x+(-32)) degF + stdtemp ; (tempF+(-stdtemp))/degF + 32
tempfahrenheit() tempF
degfahrenheit 5|9 degC
degF 5|9 degC
degreesrankine degF # The Rankine scale has the
degrankine degreesrankine # Fahrenheit degree, but its zero
degreerankine degF # is at absolute zero.
degR degrankine
tempR degrankine
temprankine degrankine
tempreaumur(x) units=[1;K] domain=[-218.52,) range=[0,) \
x degreaumur+stdtemp ; (tempreaumur+(-stdtemp))/degreaumur
degreaumur 10|8 degC # The Reaumur scale was used in Europe and
# particularly in France. It is defined
# to be 0 at the freezing point of water
# and 80 at the boiling point. Reaumur
# apparently selected 80 because it is
# divisible by many numbers.
degK K # "Degrees Kelvin" is forbidden usage.
tempK K # For consistency
# Gas mark is implemented below but in a terribly ugly way. There is
# a simple formula, but it requires a conditional which is not
# presently supported.
#
# The formula to convert to degrees Fahrenheit is:
#
# 25 log2(gasmark) + k_f gasmark<=1
# 25 (gasmark-1) + k_f gasmark>=1
#
# k_f = 275
#
gasmark[degR] \
.0625 634.67 \
.125 659.67 \
.25 684.67 \
.5 709.67 \
1 734.67 \
2 759.67 \
3 784.67 \
4 809.67 \
5 834.67 \
6 859.67 \
7 884.67 \
8 909.67 \
9 934.67 \
10 959.67
# The Beaufort wind force scale was developed from 1805-1807 by Sir Francis
# Beaufort to categorize wind conditions at sea. It is normally defined from
# Beaufort 0, also called "Force 0," through Beaufort 12. Beaufort numbers
# 13-17 were later defined for tropical cyclones but are rarely used. The
# original Beaufort scale was qualitative and did not relate directly to wind
# speed. In 1906, George Simpson of the British Met Office fit wind-speed
# measurements to visual Beaufort estimates made from five coastal and inland
# stations in Britain. Simpson's formula was adopted by the World Meterological
# Organization in 1946 to produce a table, known as WMO Code 1100, giving mean
# (and min/max) wind speed equivalents at a height of 10 meters for each
# Beaufort number. This is the "operational" Beaufort scale that mariners
# use. Meterological and climatic researchers typically use a "scientific"
# Beaufort scale based on more recent and comprehensive fits. See Wallbrink and
# Cook, Historical Wind Speed Equivalents Of The Beaufort Scale, 1850-1950, at
# https://icoads.noaa.gov/reclaim/pdf/Hisklim13.pdf
#
beaufort_WMO1100(B) units=[1;m/s] domain=[0,17] range=[0,) \
0.836 B^3|2 m/s; (beaufort_WMO1100 s / 0.836 m)^2|3
beaufort(B) units=[1;m/s] domain=[0,17] range=[0,) \
beaufort_WMO1100(B); ~beaufort_WMO1100(beaufort)
# Units cannot handle wind chill or heat index because they are two-variable
# functions, but they are included here for your edification. Clearly these
# equations are the result of a model fitting operation.
#
# wind chill index (WCI) a measurement of the combined cooling effect of low
# air temperature and wind on the human body. The index was first defined
# by the American Antarctic explorer Paul Siple in 1939. As currently used
# by U.S. meteorologists, the wind chill index is computed from the
# temperature T (in deg F) and wind speed V (in mi/hr) using the formula:
# WCI = 0.0817(3.71 sqrt(V) + 5.81 - 0.25V)(T - 91.4) + 91.4.
# For very low wind speeds, below 4 mi/hr, the WCI is actually higher than
# the air temperature, but for higher wind speeds it is lower than the air
# temperature.
#
# heat index (HI or HX) a measure of the combined effect of heat and
# humidity on the human body. U.S. meteorologists compute the index
# from the temperature T (in deg F) and the relative humidity H (as a
# value from 0 to 1).
# HI = -42.379 + 2.04901523 T + 1014.333127 H - 22.475541 TH
# - .00683783 T^2 - 548.1717 H^2 + 0.122874 T^2 H + 8.5282 T H^2
# - 0.0199 T^2 H^2.
#
# Physical constants
#
# Basic constants
pi 3.14159265358979323846 # More digits than double
tau 2 pi # precision can handle
phi (sqrt(5)+1)/2
light c
coulombconst alpha hbar c / e^2 # Coulomb constant
k_C coulombconst # Gets overridden in CGS modes
k_C_SI alpha hbar_SI c_SI / e_SI^2
epsilon0_SI 1 / 4 pi k_C_SI # Vacuum electric permittivity
epsilon0 1 / 4 pi k_C # Also overridden in CGS modes
mu0_SI 1 / epsilon0_SI c_SI^2 # Vacuum magnetic permeability
mu0 1 / epsilon0 c^2 # Also overridden in CGS modes
Z0 4 pi k_C / c # Free space impedance
energy c^2 # Convert mass to energy
hbar h / 2 pi
hbar_SI h_SI / 2 pi
spin hbar
G_SI 6.67430e-11
G 6.67430e-11 N m^2 / kg^2 # Newtonian gravitational constant
# Physico-chemical constants
atomicmassunit_SI 1.66053906892e-27
atomicmassunit 1.66053906892e-27 kg # Unified atomic mass unit, defined as
u atomicmassunit # 1|12 of the mass of carbon 12.
amu atomicmassunit # The relationship N_A u = 1 g/mol
dalton u # is approximately, but not exactly
Da dalton # true (with the 2019 SI).
# Previously the mole was defined to
# make this relationship exact.
amu_chem 1.66026e-27 kg # 1|16 of the weighted average mass of
# the 3 naturally occurring neutral
# isotopes of oxygen
amu_phys 1.65981e-27 kg # 1|16 of the mass of a neutral
# oxygen 16 atom
molarmassconstant N_A u
gasconstant k N_A # Molar gas constant (exact)
R gasconstant
kboltzmann boltzmann
sackurtetrodeconstant 5|2 + ln((u k K / 2 pi hbar^2)^(3|2) k K / atm)
# Appears in the Sakur-Tetrode
# equation for the entropy of a
# monatomic ideal gas.
molarvolume R stdtemp / atm # Volume occupied by one mole of an
V_m molarvolume # ideal gas at STP. (exact)
loschmidt avogadro / molarvolume # Molecules per cubic meter of an
n0 loschmidt # ideal gas at STP. Loschmidt did
# work similar to Avogadro.
molarvolume_si N_A siliconlattice^3 / 8 # Volume of a mole of crystalline
# silicon. The unit cell contains 8
# silicon atoms and has a side
# length of siliconlattice.
stefanboltzmann pi^2 k^4 / 60 hbar^3 c^2 # The power per area radiated by a
sigma stefanboltzmann # blackbody at temperature T is
# given by sigma T^4. (exact)
wiendisplacement (h c/k)/4.9651142317442763 # Wien's Displacement Law gives
# the wavelength at which the
# Planck spectrum has maximum
# intensity. The relation is lambda
# T = b where lambda is wavelength,
# T is temperature and b is the Wien
# displacement. This relation is
# used to determine the temperature
# of stars. The constant is the
# solution to x=5(1-exp(-x)).
# This expression has no experimental
# error, and x is defined exactly
# by the equation above, so it is
# an exact definition.
wienfrequencydisplacement 2.8214393721220788934 k/h # In a similar vein,
# this variant gives the frequency of
# maximum intensity. The constant
# is the solution to x=3*(1-exp(-x)),
# and, as above, this relation is
# an exact definition with zero
# experimental error.
K_J90 483597.9 GHz/V # Direct measurement of the volt is difficult. Until
K_J 2e/h # recently, laboratories kept Weston cadmium cells as
# a reference, but they could drift. In 1987 the
# CGPM officially recommended the use of the
# Josephson effect as a laboratory representation of
# the volt. The Josephson effect occurs when two
# superconductors are separated by a thin insulating
# layer. A "supercurrent" flows across the insulator
# with a frequency that depends on the potential
# applied across the superconductors. This frequency
# can be very accurately measured. The Josephson
# constant K_J relates the measured frequency to the
# potential. Two values given, the conventional
# (exact) value from 1990, which was used until the
# 2019 SI revision, and the current exact value.
R_K90 25812.807 ohm # Measurement of the ohm also presents difficulties.
R_K h/e^2 # The old approach involved maintaining resistances
# that were subject to drift. The new standard is
# based on the Hall effect. When a current carrying
# ribbon is placed in a magnetic field, a potential
# difference develops across the ribbon. The ratio
# of the potential difference to the current is
# called the Hall resistance. Klaus von Klitzing
# discovered in 1980 that the Hall resistance varies
# in discrete jumps when the magnetic field is very
# large and the temperature very low. This enables
# accurate realization of the resistance h/e^2 in the
# lab. The 1990 value was an exact conventional
# value used until the SI revision in 2019. This value
# did not agree with measurements. The new value
# is exact.
# The 2019 update to SI gives exact definitions for R_K and K_J. Previously
# the electromagnetic units were realized using the 1990 conventional values
# for these constants, and as a result, the standard definitions were in some
# sense outside of SI. The revision corrects this problem. The definitions
# below give the 1990 conventional values for the electromagnetic units in
# terms of 2019 SI.
ampere90 (K_J90 R_K90 / K_J R_K) A
coulomb90 (K_J90 R_K90 / K_J R_K) C
farad90 (R_K90/R_K) F
henry90 (R_K/R_K90) H
ohm90 (R_K/R_K90) ohm
volt90 (K_J90/K_J) V
watt90 (K_J90^2 R_K90 / K_J^2 R_K) W
# Various conventional values
gravity 9.80665 m/s^2 # std acceleration of gravity (exact)
# Established by the 3rd CGPM in
# 1901. This is a nominal midrange
# value, originally based on the
# acceleration of a body at sea
# level at 45 degrees latitude.
# The value was actually determined
# by measuring at the International
# Bureau and correcting the
# measurement by a theoretical
# cofficient to get the 45 deg
# latitude sea level value.
# (Wikipedia: Standard gravity)
force gravity # use to turn masses into forces
atm 101325 Pa # Standard atmospheric pressure
atmosphere atm
Hg 13.5951 gram force / cm^3 # Standard weight of mercury (exact)
water gram force/cm^3 # Standard weight of water (exact)
waterdensity gram / cm^3 # Density of water
H2O water
wc water # water column
mach 331.46 m/s # speed of sound in dry air at STP
standardtemp 273.15 K # standard temperature
stdtemp standardtemp
normaltemp tempF(70) # for gas density, from NIST
normtemp normaltemp # Handbook 44
# Weight of mercury and water at different temperatures using the standard
# force of gravity.
Hg10C 13.5708 force gram / cm^3 # These units, when used to form
Hg20C 13.5462 force gram / cm^3 # pressure measures, are not accurate
Hg23C 13.5386 force gram / cm^3 # because of considerations of the
Hg30C 13.5217 force gram / cm^3 # revised practical temperature scale.
Hg40C 13.4973 force gram / cm^3
Hg60F 13.5574 force gram / cm^3
H2O0C 0.99987 force gram / cm^3
H2O5C 0.99999 force gram / cm^3
H2O10C 0.99973 force gram / cm^3
H2O15C 0.99913 force gram / cm^3
H2O18C 0.99862 force gram / cm^3
H2O20C 0.99823 force gram / cm^3
H2O25C 0.99707 force gram / cm^3
H2O50C 0.98807 force gram / cm^3
H2O100C 0.95838 force gram / cm^3
# Atomic constants
hartree 4.3597447222060e-18 J # Approximate electric potential energy
E_h hartree # of the hydrogen atom in its ground
# state, and approximately twice its
# ionization energy. The hartree
# energy is traditionally defined as
# coulombconst^2 m_e e^4 / hbar^2,
# but it can be measured to greater
# precision using the relationship
# hartree = 2 h c Rinfinity
# because Rinfinity is one of the
# most accurately measured physical
# constants. Because h and c are
# exact we can choose either hartree
# or Rinfinity from CODATA to use as
# the primary value without
# affecting the precision.
Rinfinity hartree / 2 h c # The wavelengths of a spectral series
R_H Rinfinity m_p / (m_e + m_p) # can be expressed as
# 1/lambda = R (1/m^2 - 1/n^2).
# where R is a number that various
# slightly from element to element.
# For hydrogen, R_H is the value,
# and for heavy elements, the value
# approaches Rinfinity, which can be
# computed from
# Rinfinity = m_e c alpha^2 / 2 h
# with loss of precision. Rinfinity
# is one of the most accurately
# measured physical constants and is
# known to higher precision than m_e
# or alpha.
alpha 7.2973525643e-3 # The fine structure constant was
# introduced to explain fine
# structure visible in spectral
# lines.
bohrradius hbar / alpha m_e c
a0 bohrradius
prout 185.5 keV # nuclear binding energy equal to 1|12
# binding energy of the deuteron
conductancequantum e^2 / pi hbar
G0 conductancequantum
magneticfluxquantum pi hbar / e
Phi0 magneticfluxquantum
circulationquantum h / 2 m_e
# weak-force related
weakmixingangle 0.22305
w_to_z_mass_ratio 0.88145
# Particle radius
electronradius alpha^2 bohrradius # Classical
thomsoncrosssection 8|3 pi electronradius^2 # Arises in Thomson scattering
alphachargeradius 1.6785e-15 m
deuteronchargeradius 2.12778e-15 m
protonchargeradius 8.4075e-16 m
# Masses of elementary particles
electronmass_SI electronmass_u atomicmassunit_SI
electronmass_u 5.485799090441e-4
electronmass 5.485799090441e-4 u
m_e electronmass
muonmass 0.1134289257 u
m_mu muonmass
taumass 1.90754 u
m_tau taumass
protonmass 1.0072764665789 u
m_p protonmass
neutronmass 1.00866491606 u
m_n neutronmass
deuteronmass 2.013553212544 u # Nucleus of deuterium, one
m_d deuteronmass # proton and one neutron
alphaparticlemass 4.001506179129 u # Nucleus of He, two protons
m_alpha alphaparticlemass # and two neutrons
tritonmass 3.01550071597 u # Nucleus of H3, one proton
m_t tritonmass # and two neutrons
helionmass 3.014932246932 u # Nucleus of He3, two protons
m_h helionmass # and one neutron
# particle wavelengths: the compton wavelength of a particle is
# defined as h / m c where m is the mass of the particle.
electronwavelength h / m_e c
lambda_C electronwavelength
protonwavelength h / m_p c
lambda_C,p protonwavelength
neutronwavelength h / m_n c
lambda_C,n neutronwavelength
muonwavelength h / m_mu c
lambda_C,mu muonwavelength
tauwavelength h / m_tau c
lambda_C,tau tauwavelength
# The g-factor or dimensionless magnetic moment is a quantity that
# characterizes the magnetic moment of a particle. The electron g-factor is
# one of the most precisely measured values in physics, with a relative
# uncertainty of 1.7e-13.
g_d 0.8574382335 # Deuteron g-factor
g_e -2.00231930436092 # Electron g-factor
g_h -4.2552506995 # Helion g-factor
g_mu -2.00233184123 # Muon g-factor
g_n -3.82608552 # Neutron g-factor
g_p 5.5856946893 # Proton g-factor
g_t 5.957924930 # Triton g-factor
fermicoupling 1.1663787e-5 / GeV^2
# Magnetic moments (derived from the more accurate g-factors)
#
# The magnetic moment is g * mu_ref * spin where in most cases
# the reference is the nuclear magneton, and all of the particles
# except the deuteron have spin 1/2.
bohrmagneton e hbar / 2 electronmass # Reference magnetic moment for
mu_B bohrmagneton # the electron
mu_e g_e mu_B / 2 # Electron spin magnet moment
mu_mu g_mu mu_B m_e / 2 muonmass # Muon spin magnetic moment
nuclearmagneton mu_B m_e / protonmass # Convenient reference magnetic
mu_N nuclearmagneton # moment for heavy particles
mu_p g_p mu_N / 2 # Proton magnetic moment
mu_n g_n mu_N / 2 # Neutron magnetic moment
mu_d g_d mu_N # Deuteron magnetic moment, spin 1
mu_t g_t mu_N / 2 # Triton magnetic moment
mu_h g_h mu_N / 2 # Helion magnetic moment
shielded_mu_h -1.07455311035e-26 J / T
shielded_mu_p 1.4105705830e-26 J / T
#
# Units derived from physical constants
#
kgf kg force
technicalatmosphere kgf / cm^2
at technicalatmosphere
hyl kgf s^2 / m # Also gram-force s^2/m according to [15]
mmHg mm Hg
torr atm / 760 # The torr, named after Evangelista
# Torricelli, and is very close to the mm Hg
tor Pa # Suggested in 1913 but seldom used [24].
# Eventually renamed the Pascal. Don't
# confuse the tor with the torr.
inHg inch Hg
inH2O inch water
mmH2O mm water
eV e V # Energy acquired by a particle with charge e
electronvolt eV # when it is accelerated through 1 V
lightyear c julianyear # The 365.25 day year is specified in
ly lightyear # NIST publication 811
lightsecond c s
lightminute c min
parsec au / tan(arcsec) # Unit of length equal to distance
pc parsec # from the Sun to a point having
# heliocentric parallax of 1
# arcsec (derived from parallax
# second). A distant object with
# parallax theta will be about
# (arcsec/theta) parsecs from the
# Sun (using the approximation
# that tan(theta) = theta).
rydberg 1|2 hartree # Rydberg energy
crith 0.089885 gram # The crith is the mass of one
# liter of hydrogen at standard
# temperature and pressure.
amagat N_A / molarvolume # Used to measure gas as a number
amagatvolume mol molarvolume # density
lorentz bohrmagneton / h c # Used to measure the extent
# that the frequency of light
# is shifted by a magnetic field.
cminv h c / cm # Unit of energy used in infrared
invcm cminv # spectroscopy.
wavenumber 1/cm #
kcal_mol kcal_th / mol N_A # kcal/mol is used as a unit of
# energy by physical chemists.
#
# CGS system based on centimeter, gram and second
#
dyne cm gram / s^2 # force
dyn dyne
erg cm dyne # energy
poise gram / cm s # viscosity, honors Jean Poiseuille
P poise
rhe /poise # reciprocal viscosity
stokes cm^2 / s # kinematic viscosity
St stokes
stoke stokes
lentor stokes # old name
Gal cm / s^2 # acceleration, used in geophysics
galileo Gal # for Earth's gravitational field
# (note that "gal" is for gallon
# but "Gal" is the standard symbol
# for the gal which is evidently a
# shortened form of "galileo".)
barye dyne/cm^2 # pressure
barad barye # old name
kayser 1/cm # Proposed as a unit for wavenumber
balmer kayser # Even less common name than "kayser"
kine cm/s # velocity
bole g cm / s # momentum
pond gram force
glug gram force s^2 / cm # Mass which is accelerated at
# 1 cm/s^2 by 1 gram force
darcy centipoise cm^2 / s atm # Measures permeability to fluid flow.
# One darcy is the permeability of a
# medium that allows a flow of cc/s
# of a liquid of centipoise viscosity
# under a pressure gradient of
# atm/cm. Named for H. Darcy.
mobileohm cm / dyn s # mobile ohm, measure of mechanical
# mobility
mechanicalohm dyn s / cm # mechanical resistance
acousticalohm dyn s / cm^5 # ratio of the sound pressure of
# 1 dyn/cm^2 to a source of strength
# 1 cm^3/s
ray acousticalohm
rayl dyn s / cm^3 # Specific acoustical resistance
eotvos 1e-9 Gal/cm # Change in gravitational acceleration
# over horizontal distance
#
# Electromagnetic CGS Units
#
# For measuring electromagnetic quantities in SI, we introduce the new base
# dimension of current, define the ampere to measure current, and derive the
# other electromagnetic units from the ampere. With the CGS units one approach
# is to use the basic equations of electromagnetism to define units that
# eliminate constants from those equations. Coulomb's law has the form
#
# F = k_C q1 q2 / r^2
#
# where k_C is the Coulomb constant equal to 1|4 pi epsilon0 in SI units.
# Ampere's force law takes the form
#
# dF/dl = 2 k_A I1 I2 / r
#
# where k_A is the ampere constant. In the CGS system we force either k_C or
# k_A to 1 which then defines either a unit for charge or a unit for current.
# The other unit then becomes a derived unit. When k_C is 1 the ESU system
# results. When k_A is 1 the EMU system results. Note that these parameters
# are not independent of each other: Maxwell's equations indicate that
#
# k_C / k_A = c^2
#
# where c is the speed of light.
#
# One more choice is needed to define a complete system. Using Coulomb's law
# we define the electric field as the force per unit charge
#
# E = k_C 1 / r^2.
#
# But what about the magnetic field? It is derived from Ampere's law but we
# have the option of adding a proportionality constant, k_B, that may have
# dimensions:
#
# B = 2 k_A k_B I / r
#
# We can choose k_B = 1, which is done in the SI, ESU and EMU systems. But if
# instead we give k_B units of length/time then the magnetic field has
# the same units as the electric field. This choice leads to the Gaussian
# and Heaviside-Lorentz systems.
#
# The relations above are used to determine the dimensions, but the units are
# derived from the base units of CGS, not directly from those formulas. We
# will use the notation [unit] to refer to the dimension of the unit in
# brackets. This same process gives rise to the SI units such as the tesla,
# which is defined by
#
# [tesla] = [2 (1/4 pi c^2 epsilon0) amp / m] = [(mu0 / 2) amp / m]
#
# which gives kg / A s^2 as expected.
#
# References:
#
# Classical Electrodynamics by John David Jackson, 3rd edition.
# Cardarelli, Francois. 1999. Scientific Unit Conversion. 2nd ed. Trans.
# M.J. Shields. London: Springer-Verlag. ISBN 1-85233-043-0
#
#
# All of the CGS systems result in electromagnetic units that involve the square
# roots of the centimeter and gram. This requires a change in the primitive
# units.
#
!var UNITS_SYSTEM esu emu gaussian gauss hlu
sqrt_cm !
sqrt_centimeter sqrt_cm
+m 100 sqrt_cm^2
sqrt_g !
sqrt_gram sqrt_g
+kg kilo sqrt_g^2
!endvar
# Electrostatic CGS (ESU)
#
# This system uses the statcoulomb as the fundamental unit of charge, with
# derived units that parallel the conventional terminology but use the stat-
# prefix. The statcoulomb is derived from Coulomb's law based on the dyne
#
# dyne = statcoulomb^2 / k_C cm^2.
#
# and in the EUS system, k_C=1. The statcoulomb is also called the
# franklin or esu.
#
# The ESU system was specified by a committee report in 1873 and rarely used.
statcoulomb sqrt(dyne cm^2/k_C) # Charge such that two charges
esu statcoulomb # of 1 statC separated by 1 cm
statcoul statcoulomb # exert a force of 1 dyne
statC statcoulomb
stC statcoulomb
franklin statcoulomb
Fr franklin
!var UNITS_SYSTEM esu
!message CGS-ESU units selected
!prompt (ESU)
+coulombconst 1
+epsilon0 1 / k_C # SI relation: 1 / 4 pi k_C
+A 10 c_SI statamp
!endvar
statampere statcoulomb / s
statamp statampere
statA statampere
stA statampere
statvolt dyne cm / statamp sec
statV statvolt
stV statvolt
statfarad statamp sec / statvolt
statF statfarad
stF statfarad
cmcapacitance statfarad
stathenry statvolt sec / statamp
statH stathenry
stH stathenry
statohm statvolt / statamp
stohm statohm
statmho /statohm
stmho statmho
statweber statvolt sec
statWb statweber
stWb statweber
stattesla statWb/cm^2 # Defined by analogy with SI; rarely
statT stattesla # if ever used
stT stattesla
debye 1e-10 statC angstrom # unit of electrical dipole moment
helmholtz debye/angstrom^2 # Dipole moment per area
jar 1000 statfarad # approx capacitance of Leyden jar
# Electromagnetic CGS (EMU)
#
# The abampere is the fundamental unit of this system, with the derived units
# using the ab- prefix. The dimensions of the abampere are defined by assuming
# that k_A=1, which
#
# [dyne / cm] = [2 abampere^2 / cm]
#
# where the brackets indicate taking the dimension of the unit in base units
# and discarding any constant factors. This results in the definition from
# base CGS units of:
#
# abampere = sqrt(dyne).
#
# The abampere is also called the biot. The magnetic field unit (the gauss)
# follows from the assumption that k_B=1, which means
#
# B = 2 I / r,
#
# and hence the dimensions of the gauss are given by
#
# [gauss] = [2 abampere / cm]
#
# or rewriting in terms of the base units
#
# gauss = abampere / cm.
#
# The definition given below is different because it is in a form that
# gives a valid reduction for SI and ESU and still gives the correct
# result in EMU. (It can be derived from Faraday's law.)
#
# The EMU system was developed by Gauss and Weber and formalized as a system in
# a committee report by the British Association for the Advancement of Science
# in 1873.
abampere 10 A # Current which produces a force of
abamp abampere # 2 dyne/cm between two infinitely
aA abampere # long wires that are 1 cm apart
abA abampere
biot abampere
Bi biot
!var UNITS_SYSTEM emu
!message CGS-EMU units selected
!prompt (EMU)
+coulombconst c^2
+epsilon0 1 / k_C # SI relation: 1 / 4 pi k_C
+abampere sqrt(dyne)
+A 0.1 abamp
!endvar
abcoulomb abamp sec
abcoul abcoulomb
abC abcoulomb
abfarad abampere sec / abvolt
abF abfarad
abhenry abvolt sec / abamp
abH abhenry
abvolt dyne cm / abamp sec
abV abvolt
abohm abvolt / abamp
abmho /abohm
maxwell erg / abamp # Also called the "line"
Mx maxwell
gauss maxwell / cm^2 # The magnetic field 2 cm from a wire
Gs gauss # carrying a current of 1 abampere
oersted gauss / mu0 # From the relation H = B / mu
Oe oersted
gilbert gauss cm / mu0
Gb gilbert
Gi gilbert
unitpole 4 pi maxwell # unit magnetic pole
emu erg/gauss # "electro-magnetic unit", a measure of
# magnetic moment, often used as emu/cm^3
# to specify magnetic moment density.
# Electromagnetic CGS (Gaussian)
#
# The Gaussian system uses the statcoulomb and statamp from the ESU system
# derived by setting k_C=1, but it defines the magnetic field unit differently
# by taking k_B=c instead of k_B=1. As noted above, k_C and k_A are not
# independent. With k_C=1 we must have k_A=c^-2. This results in the magnetic
# field unit, the gauss, having dimensions give by:
#
# [gauss] = [2 (c^-2) c statamp / cm] = [statamp / c cm]
#
# We then define the gauss using base CGS units to obtain
#
# gauss = statamp / ((cm/s) cm) = statcoulomb / cm^2.
#
# Note that this definition happens to give the same result as the definition
# for the EMU system, so the definitions of the gauss are consistent.
#
# This definition gives the same dimensions for the E and B fields and was also
# known as the "symmetric system". This system was proposed by Hertz in 1888.
!var UNITS_SYSTEM gaussian gauss
!message CGS-Gaussian units selected
!prompt (Gaussian)
!endvar
!var UNITS_SYSTEM gaussian gauss natural-gauss
+coulombconst 1
+A 10 c_SI statamp
# Some SI-based definitions need re-scaling
# by factors of "c" and/or "4 pi":
+epsilon0 1 / k_C # SI relation: 1 / 4 pi k_C
+mu0 1 / epsilon0 # SI relation: 1 / epsilon0 c^2
+bohrmagneton (e hbar / 2 electronmass) / c
+magneticfluxquantum c (pi hbar / e)
+maxwell c (erg / abamp)
+weber c (J / A)
!endvar
# Electromagnetic CGS (Heaviside-Lorentz)
# The Heaviside-Lorentz system is similar to the Gaussian system, but it is
# "rationalized" so that factors of 4 pi do not appear in Maxwell's equations.
# The SI system is similarly rationalized, but the other CGS systems are not.
#
# The factor of 4 pi appears instead in Coulomb's law, so in this system
# k_C = 1 / 4 pi, which means the charge unit is defined by
#
# dyne = (1 / 4 pi) hlu_charge^2 / cm^2.
#
# Since we have the leading constant of (1 / 4pi) the numerical value of the
# charge number is larger by sqrt(4pi), which in turns means that the HLU
# charge unit is smaller by this multiple. But note that the dimensions of the
# charge unit are the same as the Gaussian system, so both systems measure
# charge with cm^(3/2) g^(1/2) / s, but the amount of charge for this dimension
# differs by a factor of sqrt(4pi) between the two systems.
#
# Ampere's law for the Heaviside-Lorentz system has the form
#
# B = 1/(2 pi c) * I/r
# The Heaviside-Lorentz system does not appear to have any named units, so we
# use "hlu" for "Heaviside-Lorentz unit" so we can define values for the basic
# units in this system.
hlu_charge statcoulomb / sqrt(4 pi)
hlu_current hlu_charge / sec
hlu_volt erg / hlu_charge
hlu_efield hlu_volt / cm
hlu_bfield sqrt(4 pi) gauss
!var UNITS_SYSTEM hlu
!message CGS-Heaviside-Lorentz Units selected
!prompt (HLU)
!endvar
!var UNITS_SYSTEM hlu natural planck planck-red
+coulombconst 1 / 4 pi
+A 10 c_SI statamp
# Some SI-based magnetism definitions
# need re-scaling by factors of "c":
+mu0 1 / epsilon0 # SI relation: 1 / epsilon0 c^2
+bohrmagneton (e hbar / 2 electronmass) / c
+magneticfluxquantum c (pi hbar / e)
+weber c (J / A)
+maxwell c (erg / abamp)
!endvar
# "Natural units" (high energy physics and cosmology)
#
# In particle physics "natural units" (which don't seem to have a more specific
# name) are defined by setting hbar = c = boltzmann = 1. In this system the
# electron volt is the only base unit. The electromagnetic units can be
# derived from the rationalized Heaviside-Lorentz units or from Gaussian units.
# The default form is the rationalized HLU derived version.
#
# The basic mechanical and thermodynamic definitions for the natural
# units are identical in both systems. These appear below. The
# natural-gauss system has additional electromagnetic redefinitions
# that appear above in the "Electromagnetic CGS (Gaussian)" Section.
# These are the Heaviside-Lorentz natural units
natural_action hbar
natural_energy eV #XXX according to CODATA 2022 (at least), natural energy = m_e c^2
natural_charge e / sqrt(4 pi alpha)
natural_time natural_action / natural_energy
natural_length natural_time c
natural_mass natural_energy / c^2
natural_momentum natural_energy / c
natural_temp natural_energy / boltzmann
natural_force natural_energy / natural_length
natural_power natural_energy / natural_time
natural_volt natural_energy / natural_charge
natural_Efield natural_volt / natural_length
natural_Bfield natural_Efield / c
natural_current natural_charge / natural_time
!var UNITS_SYSTEM natural
!message Natural units selected (Heavyside-Lorentz based)
!prompt (natural)
!endvar
!var UNITS_SYSTEM natural-gauss
!message Natural units selected (Gaussian based)
!prompt (natgauss)
!endvar
# These definitions are the same in both natural unit systems
!var UNITS_SYSTEM natural natural-gauss
+eV !
+h 2 pi
+c 1
+boltzmann 1
+m e_SI / hbar_SI c_SI eV
+kg (c_SI^2 / e_SI) eV
+s e_SI / hbar_SI eV
+K (k_SI / e_SI) eV
!endvar
#
# Planck units
#
# Planck units are a set of "natural" units based on physical constants c, G,
# hbar, boltzmann's constant, and epsilon0, often used when working with
# gravitational theory. In planck units, all quantities are dimensionless.
# Some variations are possible for exactly how the units are defined. We
# provide two variations, the rationalized planck units and the
# rationalized-reduced planck units.
#
# In both forms the units are defined by c = hbar = boltzmann = 1.
# But the choice of rationalized and reduced affects how epsilon0 and G
# are treated.
#
# In the "rationalized" units, factors of 4 pi do not appear in Maxwell's
# equation, and Coulomb's law bears a factor of 1/4 pi. See the section on
# the Heaviside-Lorentz units for more about this. The choice of rationalized
# units means that epsilon0 = 1. (In the unrationalized case, which is not
# supported, 1/(4 pi epsilon0) = 1.)
#
# The "reduced" units similarly are defined to eliminate factors of 8 pi
# from the Einstein field equations for gravitation. With reduced units
# we set 8 pi G = 1 and with the unreduced units, simply G = 1.
# Rationalized, unreduced planck units
planckmass sqrt(hbar c / G)
m_P planckmass
planckenergy planckmass c^2
E_P planckenergy
plancktime hbar / planckenergy
t_P plancktime
plancklength plancktime c
l_P plancklength
plancktemperature planckenergy / k
T_P plancktemperature
planckforce planckenergy / plancklength
planckcharge sqrt(epsilon0 hbar c)
planckcurrent planckcharge / plancktime
planckvolt planckenergy / planckcharge
planckEfield planckvolt / plancklength
planckBfield planckEfield / c
# Rationalized, reduced planck units
planckmass_red sqrt(hbar c / 8 pi G)
planckenergy_red planckmass_red c^2
plancktime_red hbar / planckenergy_red
plancklength_red plancktime_red c
plancktemperature_red planckenergy_red / k
planckforce_red planckenergy_red / plancklength_red
planckcharge_red sqrt(epsilon0 hbar c)
planckcurrent_red planckcharge_red / plancktime_red
planckvolt_red planckenergy_red / planckcharge_red
planckEfield_red planckvolt_red / plancklength_red
planckBfield_red planckEfield_red /c
!var UNITS_SYSTEM planck
!message Planck units selected
!prompt (planck)
+c 1
+h 2 pi
+G 1
+boltzmann 1
+kg sqrt(G_SI / hbar_SI c_SI)
+s c_SI^2 / hbar_SI kg
+m s / c_SI
+K k_SI / hbar_SI s
!endvar
!var UNITS_SYSTEM planck-red
!message Reduced planck units selected
!prompt (planck reduced)
+c 1
+h 2 pi
+G 1/8 pi
+boltzmann 1
+kg sqrt(8 pi G_SI / hbar_SI c_SI)
+s c_SI^2 / hbar_SI kg
+m s / c_SI
+K k_SI / hbar_SI s
!endvar
#
# Some historical electromagnetic units
#
intampere 0.999835 A # Defined as the current which in one
intamp intampere # second deposits .001118 gram of
# silver from an aqueous solution of
# silver nitrate.
intfarad 0.999505 F
intvolt 1.00033 V
intohm 1.000495 ohm # Defined as the resistance of a
# uniform column of mercury containing
# 14.4521 gram in a column 1.063 m
# long and maintained at 0 degC.
daniell 1.042 V # Meant to be electromotive force of a
# Daniell cell, but in error by .04 V
faraday N_A e mol # Charge that must flow to deposit or
faraday_phys 96521.9 C # liberate one gram equivalent of any
faraday_chem 96495.7 C # element. (The chemical and physical
faradayconst N_A e # values are off slightly from what is
# obtained by multiplying by amu_chem
# or amu_phys. These values are from
# a 1991 NIST publication.) Note that
# there is also a Faraday constant,
# which has units of C/mol.
kappline 6000 maxwell # Named by and for Gisbert Kapp
siemensunit 0.9534 ohm # Resistance of a meter long column of
# mercury with a 1 mm cross section.
#
# Printed circuit board units.
#
# Iowa State University Center for Nondestructive Evaluation
# Electrical Conductivity and Resistivity
# https://www.nde-ed.org/Physics/Materials/Physical_Chemical/Electrical.xhtml
#
# Conductivity is often expressed as a percentage of IACS. A copper wire a
# meter long with a 1 mm^2 cross section has a resistance of 1|58 ohm at
# 20 deg C. Copper density also has a standard IACS value at that temperature.
#
copperconductivity 58 siemens m / mm^2 # A wire a meter long with
IACS copperconductivity # a 1 mm^2 cross section
copperdensity 8.89 g/cm^3 # The "ounce" measures the
ouncecopper oz / ft^2 copperdensity # thickness of copper used
ozcu ouncecopper # in circuitboard fabrication
#
# Photometric units
#
LUMINOUS_INTENSITY candela
LUMINOUS_FLUX lumen
LUMINOUS_ENERGY talbot
ILLUMINANCE lux
EXITANCE lux
candle 1.02 candela # Standard unit for luminous intensity
hefnerunit 0.9 candle # in use before candela
hefnercandle hefnerunit #
violle 20.17 cd # luminous intensity of 1 cm^2 of
# platinum at its temperature of
# solidification (2045 K)
lumen cd sr # Luminous flux (luminous energy per
lm lumen # time unit)
talbot lumen s # Luminous energy
lumberg talbot # References give these values for
lumerg talbot # lumerg and lumberg both. Note that
# a paper from 1948 suggests that
# lumerg should be 1e-7 talbots so
# that lumergs/erg = talbots/joule.
# lumerg = luminous erg
lux lm/m^2 # Illuminance or exitance (luminous
lx lux # flux incident on or coming from
phot lumen / cm^2 # a surface)
ph phot #
footcandle lumen/ft^2 # Illuminance from a 1 candela source
# at a distance of one foot
metercandle lumen/m^2 # Illuminance from a 1 candela source
# at a distance of one meter
mcs metercandle s # luminous energy per area, used to
# measure photographic exposure
nox 1e-3 lux # These two units were proposed for
skot 1e-3 apostilb # measurements relating to dark adapted
# eyes.
# Luminance measures
LUMINANCE nit
nit cd/m^2 # Luminance: the intensity per projected
stilb cd / cm^2 # area of an extended luminous source.
sb stilb # (nit is from latin nitere = to shine.)
apostilb cd/pi m^2
asb apostilb
blondel apostilb # Named after a French scientist.
# Equivalent luminance measures. These units are units which measure
# the luminance of a surface with a specified exitance which obeys
# Lambert's law. (Lambert's law specifies that luminous intensity of
# a perfectly diffuse luminous surface is proportional to the cosine
# of the angle at which you view the luminous surface.)
equivalentlux cd / pi m^2 # luminance of a 1 lux surface
equivalentphot cd / pi cm^2 # luminance of a 1 phot surface
lambert cd / pi cm^2
footlambert cd / pi ft^2
# The bril is used to express "brilliance" of a source of light on a
# logarithmic scale to correspond to subjective perception. An increase of 1
# bril means doubling the luminance. A luminance of 1 lambert is defined to
# have a brilliance of 1 bril.
bril(x) units=[1;lambert] 2^(x+-100) lamberts ;log2(bril/lambert)+100
# Some luminance data from the IES Lighting Handbook, 8th ed, 1993
sunlum 1.6e9 cd/m^2 # at zenith
sunillum 100e3 lux # clear sky
sunillum_o 10e3 lux # overcast sky
sunlum_h 6e6 cd/m^2 # value at horizon
skylum 8000 cd/m^2 # average, clear sky
skylum_o 2000 cd/m^2 # average, overcast sky
moonlum 2500 cd/m^2
#
# Photographic Exposure Value
# This section by Jeff Conrad (jeff_conrad@msn.com)
#
# The Additive system of Photographic EXposure (APEX) proposed in ASA
# PH2.5-1960 was an attempt to simplify exposure determination for people who
# relied on exposure tables rather than exposure meters. Shortly thereafter,
# nearly all cameras incorporated exposure meters, so the APEX system never
# caught on, but the concept of exposure value remains in use. Though given as
# 'Ev' in ASA PH2.5-1960, it is now more commonly indicated by 'EV'. EV is
# related to exposure parameters by
#
# A^2 LS ES
# 2^EV = --- = -- = --
# t K C
#
# Where
# A = Relative aperture (f-number)
# t = Exposure time in seconds
# L = Scene luminance in cd/m2
# E = Scene illuminance in lux
# S = Arithmetic ISO speed
# K = Reflected-light meter calibration constant
# C = Incident-light meter calibration constant
#
# Strictly, an exposure value is a combination of aperture and exposure time,
# but it's also commonly used to indicate luminance (or illuminance).
# Conversion to luminance or illuminance units depends on the ISO speed and the
# meter calibration constant. Common practice is to use an ISO speed of 100.
# Calibration constants vary among camera and meter manufacturers: Canon,
# Nikon, and Sekonic use a value of 12.5 for reflected-light meters, while
# Kenko (formerly Minolta) and Pentax use a value of 14. Kenko and Sekonic use
# a value of 250 for incident-light meters with flat receptors.
#
# The values for in-camera meters apply only averaging, weighted-averaging, or
# spot metering--the multi-segment metering incorporated in most current
# cameras uses proprietary algorithms that evaluate many factors related to the
# luminance distribution of what is being metered; they are not amenable to
# simple conversions, and are usually not disclosed by the manufacturers.
s100 100 / lx s # ISO 100 speed
iso100 s100
# Reflected-light meter calibration constant with ISO 100 speed
k1250 12.5 (cd/m2) / lx s # For Canon, Nikon, and Sekonic
k1400 14 (cd/m2) / lx s # For Kenko (Minolta) and Pentax
# Incident-light meter calibration constant with ISO 100 film
c250 250 lx / lx s # flat-disc receptor
# Exposure value to scene luminance with ISO 100 imaging media
# For Kenko (Minolta) or Pentax
#ev100(x) units=[;cd/m^2] range=(0,) 2^x k1400 / s100; log2(ev100 s100/k1400)
# For Canon, Nikon, or Sekonic
ev100(x) units=[1;cd/m^2] range=(0,) 2^x k1250 / s100; log2(ev100 s100/k1250)
EV100() ev100
# Exposure value to scene illuminance with ISO 100 imaging media
iv100(x) units=[1;lx] range=(0,) 2^x c250 / s100; log2(iv100 s100 / c250)
# Other Photographic Exposure Conversions
#
# As part of APEX, ASA PH2.5-1960 proposed several logarithmic quantities
# related by
#
# Ev = Av + Tv = Bv + Sv
#
# where
# Av = log2(A^2) Aperture value
# Tv = log2(1/t) Time value
# Sv = log2(N Sx) Speed value
# Bv = log2(B S / K) Luminance ("brightness") value
# Iv = log2(I S / C) Illuminance value
#
# and
# A = Relative aperture (f-number)
# t = Exposure time in seconds
# Sx = Arithmetic ISO speed in 1/lux s
# B = luminance in cd/m2
# I = luminance in lux
# The constant N derives from the arcane relationship between arithmetic
# and logarithmic speed given in ASA PH2.5-1960. That relationship
# apparently was not obvious--so much so that it was thought necessary
# to explain it in PH2.12-1961. The constant has had several values
# over the years, usually without explanation for the changes. Although
# APEX had little impact on consumer cameras, it has seen a partial
# resurrection in the Exif standards published by the Camera & Imaging
# Products Association of Japan.
#N_apex 2^-1.75 lx s # precise value implied in ASA PH2.12-1961,
# derived from ASA PH2.5-1960.
#N_apex 0.30 lx s # rounded value in ASA PH2.5-1960,
# ASA PH2.12-1961, and ANSI PH2.7-1986
#N_apex 0.3162 lx s # value in ANSI PH2.7-1973
N_exif 1|3.125 lx s # value in Exif 2.3 (2010), making Sv(5) = 100
K_apex1961 11.4 (cd/m2) / lx s # value in ASA PH2.12-1961
K_apex1971 12.5 (cd/m2) / lx s # value in ANSI PH3.49-1971; more common
C_apex1961 224 lx / lx s # value in PH2.12-1961 (20.83 for I in
# footcandles; flat sensor?)
C_apex1971 322 lx / lx s # mean value in PH3.49-1971 (30 +/- 5 for I in
# footcandles; hemispherical sensor?)
N_speed N_exif
K_lum K_apex1971
C_illum C_apex1961
# Units for Photographic Exposure Variables
#
# Practical photography sometimes pays scant attention to units for exposure
# variables. In particular, the "speed" of the imaging medium is treated as if
# it were dimensionless when it should have units of reciprocal lux seconds;
# this practice works only because "speed" is almost invariably given in
# accordance with international standards (or similar ones used by camera
# manufacturers)--so the assumed units are invariant. In calculating
# logarithmic quantities--especially the time value Tv and the exposure value
# EV--the units for exposure time ("shutter speed") are often ignored; this
# practice works only because the units of exposure time are assumed to be in
# seconds, and the missing units that make the argument to the logarithmic
# function dimensionless are silently provided.
#
# In keeping with common practice, the definitions that follow treat "speeds"
# as dimensionless, so ISO 100 speed is given simply as '100'. When
# calculating the logarithmic APEX quantities Av and Tv, the definitions
# provide the missing units, so the times can be given with any appropriate
# units. For example, giving an exposure time of 1 minute as either '1 min' or
# '60 s' will result in Tv of -5.9068906.
#
# Exposure Value from f-number and Exposure Time
#
# Because nonlinear unit conversions only accept a single quantity,
# there is no direct conversion from f-number and exposure time to
# exposure value EV. But the EV can be obtained from a combination of
# Av and Tv. For example, the "sunny 16" rule states that correct
# exposure for a sunlit scene can achieved by using f/16 and an exposure
# time equal to the reciprocal of the ISO speed in seconds; this can be
# calculated as
#
# ~Av(16) + ~Tv(1|100 s),
#
# which gives 14.643856. These conversions may be combined with the
# ev100 conversion:
#
# ev100(~Av(16) + ~Tv(1|100 s))
#
# to yield the assumed average scene luminance of 3200 cd/m^2.
# convert relative aperture (f-number) to aperture value
Av(A) units=[1;1] domain=[-2,) range=[0.5,) 2^(A/2); 2 log2(Av)
# convert exposure time to time value
Tv(t) units=[1;s] range=(0,) 2^(-t) s; log2(s / Tv)
# convert logarithmic speed Sv in ASA PH2.5-1960 to ASA/ISO arithmetic speed;
# make arithmetic speed dimensionless
# 'Sv' conflicts with the symbol for sievert; you can uncomment this function
# definition if you don't need that symbol
#Sv(S) units=[1;1] range=(0,) 2^S / (N_speed/lx s); log2((N_speed/lx s) Sv)
Sval(S) units=[1;1] range=(0,) 2^S / (N_speed/lx s); log2((N_speed/lx s) Sval)
# convert luminance value Bv in ASA PH2.12-1961 to luminance
Bv(x) units=[1;cd/m^2] range=(0,) \
2^x K_lum N_speed ; log2(Bv / (K_lum N_speed))
# convert illuminance value Iv in ASA PH2.12-1961 to illuminance
Iv(x) units=[1;lx] range=(0,) \
2^x C_illum N_speed ; log2(Iv / (C_illum N_speed))
# convert ASA/ISO arithmetic speed Sx to ASA logarithmic speed in
# ASA PH2.5-1960; make arithmetic speed dimensionless
Sx(S) units=[1;1] domain=(0,) \
log2((N_speed/lx s) S); 2^Sx / (N_speed/lx s)
# convert DIN speed/ISO logarithmic speed in ISO 6:1993 to arithmetic speed
# for convenience, speed is treated here as if it were dimensionless
Sdeg(S) units=[1;1] range=(0,) 10^((S - 1) / 10) ; (1 + 10 log(Sdeg))
Sdin() Sdeg
# Numerical Aperture and f-Number of a Lens
#
# The numerical aperture (NA) is given by
#
# NA = n sin(theta)
#
# where n is the index of refraction of the medium and theta is half
# of the angle subtended by the aperture stop from a point in the image
# or object plane. For a lens in air, n = 1, and
#
# NA = 0.5 / f-number
#
# convert NA to f-number
numericalaperture(x) units=[1;1] domain=(0,1] range=[0.5,) \
0.5 / x ; 0.5 / numericalaperture
NA() numericalaperture
#
# convert f-number to itself; restrict values to those possible
fnumber(x) units=[1;1] domain=[0.5,) range=[0.5,) x ; fnumber
# Referenced Photographic Standards
#
# ASA PH-2.5-1960. USA Standard, Method for Determining (Monochrome,
# Continuous-Tone) Speed of Photographic Negative Materials.
# ASA PH2.12-1961. American Standard, General-Purpose Photographic
# Exposure Meters (photoelectric type).
# ANSI PH3.49-1971. American National Standard for general-purpose
# photographic exposure meters (photoelectric type).
# ANSI PH2.7-1973. American National Standard Photographic Exposure Guide.
# ANSI PH2.7-1986. American National Standard for Photography --
# Photographic Exposure Guide.
# CIPA DC-008-2010. Exchangeable image file format for digital still
# cameras: Exif Version 2.3
# ISO 6:1993. International Standard, Photography -- Black-and-white
# pictorial still camera negative film/process systems --
# Determination of ISO Speed.
#
# Astronomical time measurements
#
# Astronomical time measurement is a complicated matter. The length of the
# true day at a given place can be 21 seconds less than 24 hours or 30 seconds
# over 24 hours. The two main reasons for this are the varying speed of
# Earth in its elliptical orbit and the fact that the Sun moves on the ecliptic
# instead of along the celestial equator. To devise a workable system for time
# measurement, Simon Newcomb (1835-1909) used a fictitious "mean Sun".
# Consider a first fictitious Sun traveling along the ecliptic at a constant
# speed and coinciding with the true Sun at perigee and apogee. Then
# considering a second fictitious Sun traveling along the celestial equator at
# a constant speed and coinciding with the first fictitious Sun at the
# equinoxes. The second fictitious Sun is the "mean Sun". From this equations
# can be written out to determine the length of the mean day, and the tropical
# year. The length of the second was determined based on the tropical year
# from such a calculation and was officially used from 1960-1967 until atomic
# clocks replaced astronomical measurements for a standard of time. All of the
# values below give the mean time for the specified interval.
#
# See "Mathematical Astronomy Morsels" by Jean Meeus for more details
# and a description of how to compute the correction to mean time.
#
TIME second
anomalisticyear 365.2596 days # The time between successive
# perihelion passages of
# Earth.
siderealyear 365.256360417 day # The time for Earth to make
# one revolution around the Sun
# relative to the stars.
tropicalyear 365.242198781 day # The time needed for the mean Sun
# as defined above to increase
# its longitude by 360 degrees.
# Most references defined the
# tropical year as the interval
# between vernal equinoxes, but
# this is misleading. The length
# of the season changes over time
# because of the eccentricity of
# Earth's orbit. The time
# between vernal equinoxes is
# approximately 365.24237 days
# around the year 2000. See
# "Mathematical Astronomy
# Morsels" for more details.
eclipseyear 346.62 days # The line of nodes is the
# intersection of the plane of
# Earth's orbit around the Sun
# with the plane of the Moon's
# orbit around Earth. Eclipses
# can only occur when the Moon
# and Sun are close to this
# line. The line rotates and
# appearances of the Sun on the
# line of nodes occur every
# eclipse year.
saros 223 synodicmonth # The Earth, Moon and Sun appear in
# the same arrangement every
# saros, so if an eclipse occurs,
# then one saros later, a similar
# eclipse will occur. (The saros
# is close to 19 eclipse years.)
# The eclipse will occur about
# 120 degrees west of the
# preceding one because the
# saros is not an even number of
# days. After 3 saros, an
# eclipse will occur at
# approximately the same place.
solarday day # Time from noon to noon
siderealday 86164.09054 s # The sidereal day is the interval
siderealhour 1|24 siderealday # between two successive transits
siderealminute 1|60 siderealhour # of a star over the meridian,
siderealsecond 1|60 siderealminute # or the time required for
# Earth to make one rotation
# relative to the stars. Another
# way to think about it is to
# imagine looking down at the
# solar system and noting when
# Earth has made a rotation.
# The more usual solar day is the
# time required to make a
# rotation relative to the Sun,
# which means the same point on
# Earth faces the Sun again.
# Because Earth moves in its
# orbit, it has to rotate a bit
# more to face the Sun again,
# hence the solar day is slightly
# longer than the sidereal day.
# The value given here is the
# mean day length taken from
# ssd.jpl.nasa.gov/astro_par.html
# which in turn cites the
# "Explanatory Supplement to the
# Astronomical Almanac", 1992.
anomalisticmonth 27.55454977 day # Time for the Moon to travel from
# perigee to perigee
nodicalmonth 27.2122199 day # The nodes are the points where
draconicmonth nodicalmonth # an orbit crosses the ecliptic.
draconiticmonth nodicalmonth # This is the time required to
# travel from the ascending node
# to the next ascending node.
siderealmonth 27.321661 day # Time required for the Moon to
# orbit the Earth
lunarmonth 29 days + 12 hours + 44 minutes + 2.8 seconds
# Mean time between full moons.
synodicmonth lunarmonth # Full moons occur when the Sun
lunation synodicmonth # and Moon are on opposite sides
lune 1|30 lunation # of the Earth. Since the Earth
lunour 1|24 lune # moves around the Sun, the Moon
# has to move a bit further in its
# orbit to return to the full moon
# configuration.
year tropicalyear
yr year
month 1|12 year
mo month
lustrum 5 years # The Lustrum was a Roman
# purification ceremony that took
# place every five years.
# Classically educated Englishmen
# used this term.
decade 10 years
century 100 years
millennium 1000 years
millennia millennium
solaryear year
lunaryear 12 lunarmonth
calendaryear 365 day
commonyear 365 day
leapyear 366 day
# The Julian year is The length of an average year over a 4-year cycle in the
# Julian calendar. The calendar was proposed by Julius Caesar in 46 BCE and
# took effect the following year. It has a normal year of 365 days and a leap
# year of 366 days every four years. Though this calendar was used in
# Europe for more than 1600 years, it drifts from the topical year by
# about 1 day every 128 years, which became noticeable over its period
# of use.
# This growing discrepancy between the seasons and the calendar was perhaps
# confusing but was also of concern to the Catholic Church because it led to a
# shift in the date of Easter. To correct this discrepancy, Pope Gregory XIII
# introduced the more accurate Gregorian calendar in 1582. The Gregorian year
# is the length of an average year over a 400-year cycle in the Gregorian
# calendar. Every year that is exactly divisible by four is a
# leap year, except for years that are exactly divisible by 100, unless these
# centurial years are exactly divisible by 400. This calendar was adopted by
# many Catholic countries when it was proclaimed, but was not adopted by many
# other countries until much later; Britain and the British Empire, including
# what is now the eastern part of the United States, adopted it in 1752. See
# https://en.wikipedia.org/wiki/List_of_adoption_dates_of_the_Gregorian_calendar_by_country
# for additional details.
julianyear 365.25 days
gregorianyear 365.2425 days
islamicyear 354 day # A year of 12 lunar months. They
islamicleapyear 355 day # began counting on July 16, AD 622
# when Muhammad emigrated to Medina
# (the year of the Hegira). They need
# 11 leap days in 30 years to stay in
# sync with the lunar year which is a
# bit longer than the 29.5 days of the
# average month. The months do not
# keep to the same seasons, but
# regress through the seasons every
# 32.5 years.
islamicmonth 1|12 islamicyear # They have 29 day and 30 day months.
# The Hebrew year is also based on lunar months, but synchronized to the solar
# calendar. The months vary irregularly between 29 and 30 days in length, and
# the years likewise vary. The regular year is 353, 354, or 355 days long. To
# keep up with the solar calendar, a leap month of 30 days is inserted every
# 3rd, 6th, 8th, 11th, 14th, 17th, and 19th years of a 19 year cycle. This
# gives leap years that last 383, 384, or 385 days.
#
# Planetary data from JPL's planet fact sheets. Each planet has its
# own sheet at https://nssdc.gsfc.nasa.gov/planetary/factsheet/<name>fact.html
# The source for data on the fact sheets is described at
# https://nssdc.gsfc.nasa.gov/planetary/factsheet/fact_notes.html
# and they also indicate that the values listed are not "official" values:
# there is no single set of agreed upon values.
# Sidereal days. The sidereal day is the time required for a planet to make a
# revolution relative to the stars. This is the default day value.
mercuryday mercuryday_sidereal
venusday venusday_sidereal
earthday earthday_sidereal
marsday marsday_sidereal
jupiterday jupiterday_sidereal
saturnday saturnday_sidereal
uranusday uranusday_sidereal
neptuneday neptuneday_sidereal
plutoday plutoday_sidereal
mercuryday_sidereal 1407.6 hr # Mercury is in a 3:2 resonance lock
# where it makes 3 rotations per 2 orbits
# so 3 sidereal days = 2 years
venusday_sidereal 5832.6 hr # Retrograde
earthday_sidereal siderealday
marsday_sidereal 24.6229 hr
jupiterday_sidereal 9.9250 hr
saturnday_sidereal 10.656 hr
uranusday_sidereal 17.24 hr # Retrograde
neptuneday_sidereal 16.11 hr
plutoday_sidereal 153.2928 hr # Retrograde
# In astronomy, an object's rotation is "prograde" if it rotates in
# the same direction as the primary object it orbits. Prograde
# rotation is the more common case: in Earth's solar system, Mercury,
# Earth, Mars, Jupiter, Saturn, and Neptune have prograde rotation.
# When an object rotates opposite the direction of its primary object,
# the object's rotation is "retrograde". Venus, Uranus, and Pluto have
# retrograde rotation.
#
# The solar (or synodic) day is the time from noon to noon on a planet. This
# is different from the sidereal day because the planet has moved in its orbit,
# so (if its rotation is prograde) it needs additional rotation to return to
# the same orientation relative to the Sun. In one orbital period (a year),
# this amounts to one additional complete rotation, so the number of sidereal
# days in a year is one greater than the number of solar days.
#
# If the planet's rotation is retrograde, less rotation is needed to return to
# the same orientation relative to the Sun, and the number of sidereal days in
# a year is one fewer than the number of solar days.
#
# The solar day can be computed from the sidereal day in the typical prograde
# case by:
# solar_day = sidereal_day year / (year - sidereal_day)
# If the planet's rotation is retrograde like Venus then the formula is
# solar_day = sidereal_day year / (year + sidereal_day)
# If the sidereal day and year are the same length then the same face of the
# planet faces the Sun and there is no solar day.
mercuryday_solar 4222.6 hr
venusday_solar 2802.0 hr
earthday_solar 24 hr
marsday_solar 24.6597 hr
jupiterday_solar 9.9259 hr
saturnday_solar 10.656 hr
uranusday_solar 17.24 hr
neptuneday_solar 16.11 hr
plutoday_solar 153.2820 hr
# Sidereal years
mercuryyear 87.969 day
venusyear 224.701 day
earthyear siderealyear
marsyear 686.980 day
jupiteryear 4332.589 day
saturnyear 10759.22 day
uranusyear 30685.4 day
neptuneyear 60189 day
plutoyear 90560 day
# Equatorial radii for the planets from JPL fact sheets
mercuryradius 2440.5 km
venusradius 6051.8 km
earthradius 6378.137 km
marsradius 3396.2 km
jupiterradius 71492 km # 1 bar level
saturnradius 60268 km # 1 bar level
uranusradius 25559 km # 1 bar level
neptuneradius 24764 km # 1 bar level
plutoradius 1188 km
# Volumetric mean radii
mercuryradius_mean 2440.5 km
venusradius_mean 6051.8 km
earthradius_mean 6371 km
marsradius_mean 3389.5 km
jupiterradius_mean 69911 km
saturnradius_mean 58232 km
uranusradius_mean 25362 km
neptuneradius_mean 24622 km
plutoradius_mean 1188 km
# Polar radii
mercuryradius_polar 2438.3 km
venusradius_polar 6051.8 km
marsradius_polar 3376.2 km
jupiterradius_polar 66854 km
saturnradius_polar 54364 km
uranusradius_polar 24973 km
neptuneradius_polar 24341 km
plutoradius_polar 1188 km
mercurysundist_min 46.000 Gm
mercurysundist_max 69.818 Gm
venussundist_min 107.480 Gm
venussundist_max 108.941 Gm
earthsundist_min sundist_min
earthsundist_max sundist_max
marssundist_min 206.650 Gm
marssundist_max 249.261 Gm
jupitersundist_min 740.595 Gm
jupitersundist_max 816.363 Gm
saturnsundist_min 1357.554 Gm
saturnsundist_max 1506.527 Gm
uranussundist_min 2732.696 Gm
uranussundist_max 3001.390 Gm
neptunesundist_min 4471.050 Gm
neptunesundist_max 4558.857 Gm
plutosundist_min 4434.987 Gm
plutosundist_max 7304.326 Gm
sundist 1.0000010178 au # mean Earth-Sun distance
moondist 384400 km # mean Earth-Moon distance
sundist_near 147.095 Gm # Earth-Sun distance at perihelion
sundist_min sundist_near
sundist_far 152.100 Gm # Earth-Sun distance at aphelion
sundist_max sundist_far
# The Earth-Moon distances at perigee and apogee are different for every
# lunation. The values here are the extremes for 1500-2500 according to
# Jean Meeus's Astronomical Algorithms (1991, 332).
moondist_min 356371 km # minimum distance at perigee 1500-2500
moondist_max 406720 km # maximum distance at apogee 1500-2500
# Objects on Earth are charted relative to a perfect ellipsoid whose
# dimensions are specified by different organizations. The ellipsoid is
# specified by an equatorial radius and a flattening value which defines the
# polar radius.
earthflattening IERS_earthflattening
earthradius_equatorial IERS_earthradius_equatorial
earthradius_polar (1-earthflattening) earthradius_equatorial
# The World Geodetic System maintains a standard, WGS84, which is used by the
# the GPS system. This system uses a conventional ellipsoid that was fixed in
# 1984 and has remained constant so that data collected at different times is
# referenced to the same ellipsoid. https://epsg.io/4326
WGS84_earthflattening 1|298.257223563
WGS84_earthradius_equatorial 6378137 m
WGS84_earthradius_polar (1-WGS84_earthflattening) WGS84_earthradius_equatorial
# The International Earth Rotation Service (IERS) attempts to
# maintain an accurate model of Earth, with updates to maintain the highest
# possible accuracy, even though this makes it more difficult to relate geodetic
# measurements made at different times.
# IERS Conventions, Chapter 1, General definitions and numerical standards (16 November 2017)
# https://iers-conventions.obspm.fr/content/chapter1/icc1.pdf
IERS_earthflattening 1|298.25642
IERS_earthradius_equatorial 6378136.6 m
IERS_earthradius_polar (1-IERS_earthflattening) IERS_earthradius_equatorial
landarea 148.847e6 km^2
oceanarea 361.254e6 km^2
moonradius 1738 km # mean value
sunradius 6.96e8 m
# Many astronomical values can be measured most accurately in a system of units
# using the astronomical unit and the mass of the Sun as base units. The
# uncertainty in the gravitational constant makes conversion to SI units
# significantly less accurate.
# The astronomical unit was defined to be the length of the of the semimajor
# axis of a massless object with the same year as Earth. With such a
# definition in force, and with the mass of the Sun set equal to one, Kepler's
# third law can be used to solve for the value of the gravitational constant.
# Kepler's third law says that (2 pi / T)^2 a^3 = G M where T is the orbital
# period, a is the size of the semimajor axis, G is the gravitational constant
# and M is the mass. With M = 1 and T and a chosen for Earth's orbit, we
# find sqrt(G) = (2 pi / T) sqrt(AU^3). This constant is called the Gaussian
# gravitational constant, apparently because Gauss originally did the
# calculations. However, when the original calculation was done, the value
# for the length of Earth's year was inaccurate. The value used is called
# the Gaussian year. Changing the astronomical unit to bring it into
# agreement with more accurate values for the year would have invalidated a
# lot of previous work, so instead the astronomical unit has been kept equal
# to this original value. This is accomplished by using a standard value for
# the Gaussian gravitational constant. This constant is called k.
gauss_k 0.01720209895 # This beast has dimensions of
# au^(3|2) / day and is exact.
gaussianyear (2 pi / gauss_k) days # Year that corresponds to the Gaussian
# gravitational constant. This is a
# fictional year, and doesn't
# correspond to any celestial event.
astronomicalunit 149597870700 m # IAU definition from 2012, exact
au astronomicalunit # ephemeris for the above described
# astronomical unit. (See the NASA
# site listed above.)
GMsun 132712440041.279419 km^3 / s^2 # heliocentric gravitational constant
solarmass GMsun/G # is known more accurately than G.
sunmass solarmass # Estimated from DE440
# The following are masses for planetary systems, not just the planet itself,
# except for the case of Earth, where the Moon is excluded. Masses are
# relative to G because they are known much more accurately than G.
#
# See https://ssd.jpl.nasa.gov/astro_par.html. Values are from
# the DE440 Ephemeris: https://ssd.jpl.nasa.gov/doc/Park.2021.AJ.DE440.pdf
mercurymass 22031.868551 km^3 / s^2 G
venusmass 324858.592000 km^3 / s^2 G
marsmass 42828.375816 km^3 / s^2 G
jupitermass 126712764.100000 km^3 / s^2 G
saturnmass 37940584.841800 km^3 / s^2 G
uranusmass 5794556.400000 km^3 / s^2 G
neptunemass 6836527.100580 km^3 / s^2 G
plutomass 975.500000 km^3 / s^2 G
ceresmass 62.62890 km^3 / s^2 G
vestamass 17.288245 km^3 / s^2 G
earthmass 398600.435507 km^3 / s^2 G # Earth alone
moonmass 4902.800118 km^3 / s^2 G
moonearthmassratio moonmass/earthmass
earthmoonmass earthmass+moonmass
moongravity 1.62 m/s^2
# Earth gravity values at the equator and poles. These values are
# obtained from the WGS84 model.
gravity_equatorial 9.7803263359 m / s^2
gravity_polar 9.8321849378 m / s^2
# The Hubble constant gives the speed at which distance galaxies are moving
# away from Earth according to v = H0*d, where H0 is the hubble constant
# and d is the distance to the galaxy.
hubble 70 km/s/Mpc # approximate
H0 hubble
# Parallax is the angular difference between the topocentric (on Earth's
# surface) and geocentric (at Earth's center) direction toward a celestial body
# when the body is at a given altitude. When the body is on the horizon, the
# parallax is the horizontal parallax; when the body is on the horizon and the
# observer is on the equator, the parallax is the equatorial horizontal
# parallax. When the body is at zenith, the parallax is zero.
lunarparallax asin(earthradius_equatorial / moondist) # Moon equatorial
moonhp lunarparallax # horizontal parallax
# at mean distance
# Light from celestial objects is attenuated by passage through Earth's
# atmosphere. A body near the horizon passes through much more air than an
# object at zenith, and is consequently less bright. Air mass is the ratio of
# the length of the optical path at a given altitude (angle above the horizon)
# to the length at zenith. Air mass at zenith is by definition unity; at the
# horizon, air mass is approximately 38, though the latter value can vary
# considerably with atmospheric conditions. The general formula is # E = E0
# exp(-c X), where E0 is the value outside Earth's atmosphere, E is the value
# seen by an observer, X is the air mass and c is the extinction coefficient.
# A common value for c in reasonably clear air is 0.21, but values can be
# considerably greater in urban areas. Apparent altitude is that perceived by
# an observer; it includes the effect of atmospheric refraction. There is no
# shortage of formulas for air mass
# (https://en.wikipedia.org/wiki/Air_mass_(astronomy)); all are subject to
# variations in local atmospheric conditions. The formula used here is simple
# and is in good agreement with rigorously calculated values under standard
# conditions.
#
# Extraterrestrial illuminance or luminance of an object at a given altitude
# determined with vmag() or SB_xxx() below can be multiplied by
# atm_transmission() or atm_transmissionz() to estimate the terrestrial value.
#
# Kasten and Young (1989) air mass formula. alt is apparent altitude
# Reference:
# Kasten, F., and A.T. Young. 1989. "Revised Optical Air Mass Tables
# and Approximation Formula." Applied Optics. Vol. 28, 4735-4738.
# Bibcode:1989ApOpt..28.4735K. doi:10.1364/AO.28.004735.
airmass(alt) units=[degree;1] domain=[0,90] noerror \
1 / (sin(alt) + 0.50572 (alt / degree + 6.07995)^-1.6364)
# zenith is apparent zenith angle (zenith = 90 deg - alt)
airmassz(zenith) units=[degree;1] domain=[0,90] noerror \
1 / (cos(zenith) + 0.50572 (96.07995 - zenith / degree)^-1.6364)
# For reasonably clear air at sea level; values may need adjustment for
# elevation and local atmospheric conditions
# for scotopic vision (510 nm), appropriate for the dark-adapted eye
# extinction_coeff 0.26
# for photopic vision, appropriate for observing brighter objects such
# as the full moon
extinction_coeff 0.21
atm_transmission(alt) units=[degree;1] domain=[0,90] noerror \
exp(-extinction_coeff airmass(alt))
# in terms of zenith angle (zenith = 90 deg - alt)
atm_transmissionz(zenith) units=[degree;1] domain=[0,90] noerror \
exp(-extinction_coeff airmassz(zenith))
# Moon and Sun data at mean distances
moonvmag -12.74 # Moon apparent visual magnitude at mean distance
sunvmag -26.74 # Sun apparent visual magnitude at mean distance
moonsd asin(moonradius / moondist) # Moon angular semidiameter at mean distance
sunsd asin(sunradius / sundist) # Sun angular semidiameter at mean distance
# Visual magnitude of star or other celestial object. The system of stellar
# magnitudes, developed in ancient Greece, assigned magnitudes from 1
# (brightest) to 6 (faintest visible to the naked eye). In 1856, British
# astronomer Norman Pogson made the system precise, with a magnitude 1 object
# 100 times as bright as a magnitude 6 object, and each magnitude differing
# from the next by a constant ratio; the ratio, sometimes known as Pogson's
# ratio, is thus 100^0.2, or approximately 2.5119. The logarithm of 100^0.2 is
# 0.4, hence the common use of powers of 10 and base-10 logarithms.
#
# Reference:
# Allen, C.W. 1976. Astrophysical Quantities, 3rd ed. 1973, reprinted
# with corrections, 1976. London: Athlone.
#
# The function argument is the (dimensionless) visual magnitude; reference
# illuminance of 2.54e-6 lx is from Allen (2000, 21), and is for outside
# Earth's atmosphere. Illuminance values can be adjusted to terrestrial values
# by multiplying by one of the atm_transmission functions above.
# Illuminance from apparent visual magnitude
vmag(mag) units=[1;lx] domain=[,] range=(0,] \
2.54e-6 lx 10^(-0.4 mag); -2.5 log(vmag / (2.54e-6 lx))
# Surface brightness of a celestial object of a given visual magnitude
# is a logarithmic measure of the luminance the object would have if its
# light were emitted by an object of specified solid angle; it is
# expressed in magnitudes per solid angle. Surface brightness can be
# obtained from the visual magnitude by
# S = m + 2.5 log(pi pi k a b),
# where k is the phase (fraction illuminated), a is the equatorial
# radius, and b is the polar radius. For 100% illumination (e.g., full
# moon), this is often simplified to
# S = m + 2.5 log(pi k s^2),
# where s is the object's angular semidiameter; the units of s determine
# the units of solid angle. The visual magnitude and semidiameter must
# be appropriate for the object's distance; for other than 100%
# illumination, the visual magnitude must be appropriate for the phase.
# Luminance values are for outside Earth's atmosphere; they can be
# adjusted to terrestrial values by multiplying by one of the atm_transmission
# functions above.
# luminance from surface brightness in magnitudes per square degree
SB_degree(sb) units=[1;cd/m^2] domain=[,] range=(0,] \
vmag(sb) / squaredegree ; \
~vmag(SB_degree squaredegree)
# luminance from surface brightness in magnitudes per square minute
SB_minute(sb) units=[1;cd/m^2] domain=[,] range=(0,] \
vmag(sb) / squareminute ; \
~vmag(SB_minute squareminute)
# luminance from surface brightness in magnitudes per square second
SB_second(sb) units=[1;cd/m^2] domain=[,] range=(0,] \
vmag(sb) / squaresecond ; \
~vmag(SB_second squaresecond)
# luminance from surface brightness in magnitudes per steradian
SB_sr(sb) units=[1;cd/m^2] domain=[,] range=(0,] \
vmag(sb) / sr ; \
~vmag(SB_sr sr)
SB() SB_second
SB_sec() SB_second
SB_min() SB_minute
SB_deg() SB_degree
# The brightness of one tenth-magnitude star per square degree outside
# Earth's atmosphere; often used for night sky brightness.
S10 SB_degree(10)
# Examples for magnitude and surface brightness functions
# Sun illuminance from visual magnitude
# You have: sunvmag
# You want:
# Definition: -26.74 = -26.74
# You have: vmag(sunvmag)
# You want: lx
# * 126134.45
# / 7.9280482e-06
#
# Moon surface brightness from visual magnitude and semidiameter at 100%
# illumination (full moon):
# You have: moonvmag
# You want:
# Definition: -12.74 = -12.74
# You have: moonsd
# You want: arcsec
# * 932.59484
# / 0.001072277
# You have: moonvmag + 2.5 log(pi 932.59484^2)
# You want:
# Definition: 3.3513397
#
# Similar example with specific data obtained from another source (JPL
# Horizons, https://ssd.jpl.nasa.gov/horizons.cgi); semidiameter is in
# arcseconds
#
# You have: -12.9 + 2.5 log(pi 2023.201|2^2)
# You want:
# Definition: 3.3679199
# You have: SB_second(-12.9 + 2.5 log(pi 2023.201|2^2))
# You want:
# Definition: 4858.6547 cd / m^2
#
# If surface brightness is provided by another source (e.g., Horizons),
# it can simply be used directly:
# You have: SB_second(3.3679199)
# You want: cd/m^2
# * 4858.6546
# / 0.0002058183
# The illuminance and luminance values are extraterrestrial (outside
# Earth's atmosphere). The values at Earth's surface are less than these
# because of atmospheric extinction. For example, in the last example
# above, if the Moon were at an altitude of 55 degrees, the terrestrial
# luminance could be calculated with
# You have: SB_second(3.3679199)
# You want: cd/m^2
# * 4858.6546
# / 0.0002058183
# You have: _ atm_transmission(55 deg)
# You want: cd/m^2
# * 3760.6356
# / 0.0002659125
# If desired, photographic exposure can be determined with EV100(),
# leading to acceptable combinations of aperture and exposure time.
# For the example above, but with the Moon at 10 degrees,
# You have: SB_second(3.3679199) atm_transmission(10 deg)
# You want: EV100
# 13.553962
#
# The Hartree system of atomic units, derived from fundamental units
# of mass (of the electron), action (Planck's constant), charge, and
# the Coulomb constant. This system is used in the fields of physical
# chemistry and condensed matter physics.
#
# Fundamental units
atomicmass electronmass
atomiccharge e
atomicaction hbar
atomicenergy hartree
# Derived units
atomicvelocity sqrt(atomicenergy / atomicmass)
atomictime atomicaction / atomicenergy
atomiclength atomicvelocity atomictime
atomicforce atomicenergy / atomiclength
atomicmomentum atomicenergy / atomicvelocity
atomiccurrent atomiccharge / atomictime
atomicdipolemoment atomiccharge atomiclength
atomicpotential atomicenergy / atomiccharge # electrical potential
atomicvolt atomicpotential
atomicEfield atomicpotential / atomiclength
atomicBfield atomicEfield / atomicvelocity
atomictemperature atomicenergy / boltzmann
#
# In Hartree units, m_e = hbar = e = coulombconst = bohrradius = alpha*c = 1
#
!var UNITS_SYSTEM hartree
!message Hartree units selected
!prompt (hartree)
+hartree 1
+kg 1/electronmass_SI
+K k_SI / hbar_SI s
+m alpha c_SI electronmass_SI / hbar_SI
+s alpha c_SI m
+A 1 / s e_SI
!endvar
#
# These thermal units treat entropy as charge, from [5]
#
thermalcoulomb J/K # entropy
thermalampere W/K # entropy flow
thermalfarad J/K^2
thermalohm K^2/W # thermal resistance
fourier thermalohm
thermalhenry J K^2/W^2 # thermal inductance
thermalvolt K # thermal potential difference
#
# United States units
#
# linear measure
# The US Metric Law of 1866 legalized the metric system in the USA and
# defined the meter in terms of the British system with the exact
# 1 meter = 39.37 inches. On April 5, 1893 Thomas Corwin Mendenhall,
# Superintendent of Weights and Measures, decided, in what has become
# known as the "Mendenhall Order" that the meter and kilogram would be the
# fundamental standards in the USA. The definition from 1866 was turned
# around to give an exact definition of the yard as 3600|3937 meters This
# definition was used until July of 1959 when the definition was changed
# to bring the US and other English-speaking countries into agreement; the
# Canadian value of 1 yard = 0.9144 meter (exactly) was chosen because it
# was approximately halfway between the British and US values; it had the
# added advantage of making 1 inch = 25.4 mm (exactly). Since 1959, the
# "international" foot has been exactly 0.3048 meters. At the same time,
# it was decided that any data expressed in feet derived from geodetic
# surveys within the US would continue to use the old definition and call
# the old unit the "survey foot."
#
# Until 1 January 2023, the US continued to define the statute
# mile, furlong, chain, rod, link, and fathom in terms of the US survey
# foot. Since then, use of the US survey foot has been officially
# deprecated, with its use limited to historical and legacy applications.
# These units are now defined in terms of the international foot.
#
# Sources:
# NIST Special Publication 447, Sects. 5, 7, and 8.
# NIST Handbook 44, 2024 ed., Appendix C.
# Canadian Journal of Physics, 1959, 37:(1) 84, 10.1139/p59-014.
inch 2.54 cm # Exact, international inch (1959)
in inch
foot 12 inch
feet foot
ft foot
yard 3 ft
yd yard
mile 5280 ft # The mile was enlarged from 5000 ft
# to this number in order to make
# it an even number of furlongs.
# (The Roman mile is 5000 romanfeet.)
line 1|12 inch # Also defined as '.1 in' or as '1e-8 Wb'
rod 16.5 ft
pole rod
perch rod
furlong 40 rod # From "furrow long"
statutemile mile
league 3 mile # Intended to be an hour's walk
# surveyor's measure
# The US survey foot is officially deprecated as of 1 January 2023
US 1200|3937 m/ft # These four values will convert
US- US # international measures to
survey- US # US Survey measures
geodetic- US
int 3937|1200 ft/m # Convert US Survey measures to
int- int # international measures
# values based on the US survey foot are deprecated as of 1 January 2023
surveyorschain 66 surveyft
surveychain surveyorschain
surveyorspole 1|4 surveyorschain
surveyorslink 1|100 surveyorschain
USacre 10 surveychain^2
USacrefoot USacre surveyfoot
chain 66 ft
link 1|100 chain
ch chain
intacre 10 chain^2 # Acre based on international ft
intacrefoot acre foot
acrefoot intacrefoot
acre intacre
ac acre
section mile^2
township 36 section
homestead 160 acre # Area of land granted by the 1862 Homestead
# Act of the United States Congress
gunterschain surveyorschain
engineerschain 100 ft
engineerslink 1|100 engineerschain
ramsdenschain engineerschain
ramsdenslink engineerslink
gurleychain 33 feet # Andrew Ellicott chain is the
gurleylink 1|50 gurleychain # same length
wingchain 66 feet # Chain from 1664, introduced by
winglink 1|80 wingchain # Vincent Wing, also found in a
# 33 foot length with 40 links.
# early US length standards
# The US has had four standards for the yard: one by Troughton of London
# (1815); bronze yard #11 (1856); the Mendhall yard (1893), consistent
# with the definition of the meter in the metric joint resolution of
# Congress in 1866, but defining the yard in terms of the meter; and the
# international yard (1959), which standardized definitions for Australia,
# Canada, New Zealand, South Africa, the UK, and the US.
# Sources: Pat Naughtin (2009), Which Inch?:
# https://metricationmatters.org/docs/WhichInch.pdf,
# Lewis E. Barbrow and Lewis V. Judson (1976). NBS Special
# Publication 447, Weights and Measures Standards of the United States: A
# Brief History.
troughtonyard 914.42190 mm
bronzeyard11 914.39980 mm
mendenhallyard surveyyard
internationalyard yard
# nautical measure
fathom 6 ft # Originally defined as the distance from
# fingertip to fingertip with arms fully
# extended.
nauticalmile 1852 m # Supposed to be one minute of latitude at
# the equator. That value is about 1855 m.
# Early estimates of Earth's circumference
# were a bit off. The value of 1852 m was
# made the international standard in 1929.
# The US did not accept this value until
# 1954. The UK switched in 1970.
# The cable is used for depth in water and has a wide range of definitions
intcable 1|10 nauticalmile # international cable
uscable 120 fathom # value after 1 January 2023
surveycable 120 USfathom # value before 1 January 2023
UScable surveycable
cableslength cable
cablelength cable
navycablelength cable
brcable 1|10 brnauticalmile
admiraltycable brcable
marineleague 3 nauticalmile
geographicalmile brnauticalmile
knot nauticalmile / hr
click km # US military slang
klick click
# Avoirdupois weight
pound 0.45359237 kg # Exact, International Pound (1959)
lb pound # From the Latin libra
grain 1|7000 pound # The grain is the same in all three
# weight systems. It was originally
# defined as the weight of a barley
# corn taken from the middle of the
# ear.
ounce 1|16 pound
oz ounce
dram 1|16 ounce
dr dram
ushundredweight 100 pounds
cwt hundredweight
shorthundredweight ushundredweight
uston shortton
shortton 2000 lb
quarterweight 1|4 uston
shortquarterweight 1|4 shortton
shortquarter shortquarterweight
# Troy Weight. In 1828 the troy pound was made the first United States
# standard weight. It was to be used to regulate coinage.
troypound 5760 grain
troyounce 1|12 troypound
ozt troyounce
pennyweight 1|20 troyounce # Abbreviated "d" in reference to a
dwt pennyweight # Frankish coin called the "denier"
# minted in the late 700's. There
# were 240 deniers to the pound.
assayton mg ton / troyounce # mg / assayton = troyounce / ton
usassayton mg uston / troyounce
brassayton mg brton / troyounce
fineounce troyounce # A troy ounce of 99.5% pure gold
# Some other jewelers units
metriccarat 0.2 gram # Defined in 1907
metricgrain 50 mg
carat metriccarat
ct carat
jewelerspoint 1|100 carat
silversmithpoint 1|4000 inch
momme 3.75 grams # Traditional Japanese unit based
# on the chinese mace. It is used for
# pearls in modern times and also for
# silk density. The definition here
# was adopted in 1891.
# Apothecaries' weight
appound troypound
apounce troyounce
apdram 1|8 apounce
apscruple 1|3 apdram
# Liquid measure
usgallon 231 in^3 # US liquid measure is derived from
gal gallon # the British wine gallon of 1707.
quart 1|4 gallon # See the "winegallon" entry below
pint 1|2 quart # more historical information.
gill 1|4 pint
usquart 1|4 usgallon
uspint 1|2 usquart
usgill 1|4 uspint
usfluidounce 1|16 uspint
fluiddram 1|8 usfloz
minimvolume 1|60 fluiddram
qt quart
pt pint
floz fluidounce
usfloz usfluidounce
fldr fluiddram
liquidbarrel 31.5 usgallon
usbeerbarrel 2 beerkegs
beerkeg 15.5 usgallon # Various among brewers
ponykeg 1|2 beerkeg
winekeg 12 usgallon
petroleumbarrel 42 usgallon # Originated in Pennsylvania oil
barrel petroleumbarrel # fields, from the winetierce
bbl barrel
ushogshead 2 liquidbarrel
usfirkin 9 usgallon
# Dry measures: The Winchester Bushel was defined by William III in 1702 and
# legally adopted in the US in 1836.
usbushel 2150.42 in^3 # Volume of 8 inch cylinder with 18.5
bu bushel # inch diameter (rounded)
peck 1|4 bushel
uspeck 1|4 usbushel
brpeck 1|4 brbushel
pk peck
drygallon 1|2 uspeck
dryquart 1|4 drygallon
drypint 1|2 dryquart
drybarrel 7056 in^3 # Used in US for fruits, vegetables,
# and other dry commodities except for
# cranberries.
cranberrybarrel 5826 in^3 # US cranberry barrel
heapedbushel 1.278 usbushel# The following explanation for this
# value was provided by Wendy Krieger
# <os2fan2@yahoo.com> based on
# guesswork. The cylindrical vessel is
# 18.5 inches in diameter and 1|2 inch
# thick. A heaped bushel includes the
# contents of this cylinder plus a heap
# on top. The heap is a cone 19.5
# inches in diameter and 6 inches
# high. With these values, the volume
# of the bushel is 684.5 pi in^3 and
# the heap occupies 190.125 pi in^3.
# Therefore, the heaped bushel is
# 874.625|684.5 bushels. This value is
# approximately 1.2777575 and it rounds
# to the value listed for the size of
# the heaped bushel. Sometimes the
# heaped bushel is reported as 1.25
# bushels. This same explanation gives
# that value if the heap is taken to
# have an 18.5 inch diameter.
# Grain measures. The bushel as it is used by farmers in the USA is actually
# a measure of mass which varies for different commodities. Canada uses the
# same bushel masses for most commodities, but not for oats.
wheatbushel 60 lb
soybeanbushel 60 lb
cornbushel 56 lb
ryebushel 56 lb
barleybushel 48 lb
oatbushel 32 lb
ricebushel 45 lb
canada_oatbushel 34 lb
# Wine and Spirits measure
ponyvolume 1 usfloz
jigger 1.5 usfloz # Can vary between 1 and 2 usfloz
shot jigger # Sometimes 1 usfloz
eushot 25 ml # EU standard spirits measure
fifth 1|5 usgallon
winebottle 750 ml # US industry standard, 1979
winesplit 1|4 winebottle
magnum 1.5 liter # Standardized in 1979, but given
# as 2 qt in some references
metrictenth 375 ml
metricfifth 750 ml
metricquart 1 liter
# Old British bottle size
reputedquart 1|6 brgallon
reputedpint 1|2 reputedquart
brwinebottle reputedquart # Very close to 1|5 winegallon
# French champagne bottle sizes
split 200 ml
jeroboam 2 magnum
rehoboam 3 magnum
methuselah 4 magnum
imperialbottle 4 magnum
salmanazar 6 magnum
balthazar 8 magnum
nebuchadnezzar 10 magnum
solomon 12 magnum
melchior 12 magnum
sovereign 17.5 magnum
primat 18 magnum
goliath 18 magnum
melchizedek 20 magnum
midas 20 magnum
# The wine glass doesn't seem to have an official standard, but the same value
# is suggested by several sources in the US.
wineglass 150 mL
# In the UK, serving size offerings legally mandated by The Weights and
# Measures (Specified Quantities) (Unwrapped Bread and Intoxicating
# Liquor) Order 2011, effective 1st October 2011. The quantities--not
# the names--are mandated. Lawful size offerings are these or multiples
# thereof, but other sizes can be provided at the express request of a
# buyer.
smallwineglass 125 mL
mediumwineglass 175 mL
# Values vary considerably among countries and even more so in practice. The
# "standard" US value gives 5 glasses per standard 750 ml bottle. Old practice
# in the UK was 125 ml per glass, or 6 glasses per bottle. Some sources suggest
# a more recent common value of 250 ml per glass, or 3 glasses per
# bottle; as a multiple of 125 ml, this would be a lawful serving size offering.
#
# The value refers to the size of the serving, not the total volume of the
# glass, which is typically not filled above the height of its greatest
# diameter.
#
# A unit of alcohol is a specified amount of pure ethyl alcohol, expressed as a
# mass or volumetric equivalent. Many countries use the same concept but use
# different terms. "Alcohol unit" is used officially in the UK; the US, Canada,
# and Australia use "standard drink." Values vary considerably among
# countries. The UK value of 8 g is nominally the amount of alcohol that a
# typical adult can metabolize in one hour.
alcoholunitus 14 g / ethanoldensity
alcoholunitca 13.6 g / ethanoldensity
alcoholunituk 8 g / ethanoldensity
alcoholunitau 10 g / ethanoldensity
# Common serving sizes have roughly equivalent amounts of alcohol, as
# illustrated by US examples for wine (12% Alcohol By Volume), beer (5% ABV),
# and spirits (80 proof).
#
# alcoholunitus / 12% = 147.8 mL, close to the "standard" serving of 150 mL.
# alcoholunitus / 5% = 11.995346 floz, close to a standard 12 floz bottle or can
# alcoholunitus / 80 proof = 1.4994182 floz, close to a standard "shot" or jigger
# https://www.rethinkingdrinking.niaaa.nih.gov/
# https://www.cdc.gov/alcohol/faqs.htm
# https://www.canada.ca/en/health-canada/services/substance-use/alcohol/low-risk-alcohol-drinking-guidelines
# https://www.drinkaware.co.uk/
# https://www.drinkaware.co.uk/facts/alcoholic-drinks-and-units
# https://www.gov.uk/government/uploads/system/uploads/attachment_data/file/545937/UK_CMOs__report.pdf
# https://adf.org.au/reducing-risk/alcohol/alcohol-guidelines/
# https://www.health.gov.au/topics/alcohol/about-alcohol/standard-drinks-guide
# https://en.wikipedia.org/wiki/Unit_of_alcohol
# https://en.wikipedia.org/wiki/Standard_drink
# Coffee
#
# The recommended ratio of coffee to water. Values vary considerably;
# one is from the Specialty Coffee Association of America: Brewing Best Practices
# https://sca.coffee/research/protocols-best-practices
coffeeratio 55 g/L # +/- 10%
# other recommendations are more loose, e.g.,
# http://www.ncausa.org/About-Coffee/How-to-Brew-Coffee
#
# Water is "hard" if it contains various minerals, especially calcium
# carbonate.
#
clarkdegree grains/brgallon # Content by weigh of calcium carbonate
gpg grains/usgallon # Divide by water's density to convert to
# a dimensionless concentration measure
#
# Shoe measures
#
shoeiron 1|48 inch # Used to measure leather in soles
shoeounce 1|64 inch # Used to measure non-sole shoe leather
# USA shoe sizes. These express the length of the shoe or the length
# of the "last", the form that the shoe is made on. But note that
# this only captures the length. It appears that widths change 1/4
# inch for each letter within the same size, and if you change the
# length by half a size then the width changes between 1/8 inch and
# 1/4 inch. But this may not be standard. If you know better, please
# contact me.
shoesize_delta 1|3 inch # USA shoe sizes differ by this amount
shoe_men0 8.25 inch
shoe_women0 (7+11|12) inch
shoe_boys0 (3+11|12) inch
shoe_girls0 (3+7|12) inch
shoesize_men(n) units=[1;inch] shoe_men0 + n shoesize_delta ; \
(shoesize_men+(-shoe_men0))/shoesize_delta
shoesize_women(n) units=[1;inch] shoe_women0 + n shoesize_delta ; \
(shoesize_women+(-shoe_women0))/shoesize_delta
shoesize_boys(n) units=[1;inch] shoe_boys0 + n shoesize_delta ; \
(shoesize_boys+(-shoe_boys0))/shoesize_delta
shoesize_girls(n) units=[1;inch] shoe_girls0 + n shoesize_delta ; \
(shoesize_girls+(-shoe_girls0))/shoesize_delta
# European shoe size. According to
# http://www.shoeline.com/footnotes/shoeterm.shtml
# shoe sizes in Europe are measured with Paris points which simply measure
# the length of the shoe.
europeshoesize 2|3 cm
#
# USA slang units
#
buck US$
fin 5 US$
sawbuck 10 US$
usgrand 1000 US$
greenback US$
key kg # usually of marijuana, 60's
lid 1 oz # Another 60's weed unit
footballfield usfootballfield
usfootballfield 100 yards
canadafootballfield 110 yards # And 65 yards wide
marathon 26 miles + 385 yards
#
# British
#
# The length measure in the UK was defined by a bronze bar manufactured in
# 1844. Various conversions were sanctioned for convenience at different
# times, which makes conversions before 1963 a confusing matter. Apparently
# previous conversions were never explicitly revoked. Four different
# conversion factors appear below. Multiply them times an imperial length
# units as desired. The Weights and Measures Act of 1963 switched the UK away
# from their bronze standard and onto a definition of the yard in terms of the
# meter. This happened after an international agreement in 1959 to align the
# world's measurement systems.
UK UKlength_SJJ
UK- UK
british- UK
UKlength_B 0.9143992 meter / yard # Benoit found the yard to be
# 0.9143992 m at a weights and
# measures conference around
# 1896. Legally sanctioned
# in 1898.
UKlength_SJJ 0.91439841 meter / yard # In 1922, Seers, Jolly and
# Johnson found the yard to be
# 0.91439841 meters.
# Used starting in the 1930's.
UKlength_K meter / 39.37079 inch # In 1816 Kater found this ratio
# for the meter and inch. This
# value was used as the legal
# conversion ratio when the
# metric system was legalized
# for contract in 1864.
UKlength_C meter / 1.09362311 yard # In 1866 Clarke found the meter
# to be 1.09362311 yards. This
# conversion was legalized
# around 1878.
brnauticalmile 6080 ft # Used until 1970 when the UK
brknot brnauticalmile / hr # switched to the international
admiraltymile brnauticalmile # nautical mile.
admiraltyknot brknot
seamile 6000 ft
shackle 15 fathoms # Adopted 1949 by British navy
# British Imperial weight is mostly the same as US weight. A few extra
# units are added here.
clove 7 lb
stone 14 lb
tod 28 lb
brquarterweight 1|4 brhundredweight
brhundredweight 8 stone
longhundredweight brhundredweight
longton 20 brhundredweight
brton longton
# British Imperial volume measures
brminim 1|60 brdram
brscruple 1|3 brdram
fluidscruple brscruple
brdram 1|8 brfloz
brfluidounce 1|20 brpint
brfloz brfluidounce
brgill 1|4 brpint
brpint 1|2 brquart
brquart 1|4 brgallon
brgallon 4.54609 l # The British Imperial gallon was
# defined in 1824 to be the volume of
# water which weighed 10 pounds at 62
# deg F with a pressure of 30 inHg.
# It was also defined as 277.274 in^3,
# Which is slightly in error. In
# 1963 it was defined to be the volume
# occupied by 10 pounds of distilled
# water of density 0.998859 g/ml weighed
# in air of density 0.001217 g/ml
# against weights of density 8.136 g/ml.
# This gives a value of approximately
# 4.5459645 liters, but the old liter
# was in force at this time. In 1976
# the definition was changed to exactly
# 4.54609 liters using the new
# definition of the liter (1 dm^3).
brbarrel 36 brgallon # Used for beer
brbushel 8 brgallon
brheapedbushel 1.278 brbushel
brquarter 8 brbushel
brchaldron 36 brbushel
# Obscure British volume measures. These units are generally traditional
# measures whose definitions have fluctuated over the years. Often they
# depended on the quantity being measured. They are given here in terms of
# British Imperial measures. For example, the puncheon may have historically
# been defined relative to the wine gallon or beer gallon or ale gallon
# rather than the British Imperial gallon.
bag 4 brbushel
bucket 4 brgallon
kilderkin 2 brfirkin
last 40 brbushel
noggin brgill
pottle 0.5 brgallon
pin 4.5 brgallon
puncheon 72 brgallon
seam 8 brbushel
coomb 4 brbushel
boll 6 brbushel
firlot 1|4 boll
brfirkin 9 brgallon # Used for ale and beer
cran 37.5 brgallon # measures herring, about 750 fish
brwinehogshead 52.5 brgallon # This value is approximately equal
brhogshead brwinehogshead # to the old wine hogshead of 63
# wine gallons. This adjustment
# is listed in the OED and in
# "The Weights and Measures of
# England" by R. D. Connor
brbeerhogshead 54 brgallon
brbeerbutt 2 brbeerhogshead
registerton 100 ft^3 # Used for internal capacity of ships
shippington 40 ft^3 # Used for ship's cargo freight or timber
brshippington 42 ft^3 #
freightton shippington # Both register ton and shipping ton derive
# from the "tun cask" of wine.
displacementton 35 ft^3 # Approximate volume of a longton weight of
# sea water. Measures water displaced by
# ships.
waterton 224 brgallon
strike 70.5 l # 16th century unit, sometimes
# defined as .5, 2, or 4 bushels
# depending on the location. It
# probably doesn't make a lot of
# sense to define in terms of imperial
# bushels. Zupko gives a value of
# 2 Winchester grain bushels or about
# 70.5 liters.
amber 4 brbushel# Used for dry and liquid capacity [18]
# British volume measures with "imperial"
imperialminim brminim
imperialscruple brscruple
imperialdram brdram
imperialfluidounce brfluidounce
imperialfloz brfloz
imperialgill brgill
imperialpint brpint
imperialquart brquart
imperialgallon brgallon
imperialbarrel brbarrel
imperialbushel brbushel
imperialheapedbushel brheapedbushel
imperialquarter brquarter
imperialchaldron brchaldron
imperialwinehogshead brwinehogshead
imperialhogshead brhogshead
imperialbeerhogshead brbeerhogshead
imperialbeerbutt brbeerbutt
imperialfirkin brfirkin
# obscure British lengths
barleycorn 1|3 UKinch # Given in Realm of Measure as the
# difference between successive shoe sizes
nail 1|16 UKyard # Originally the width of the thumbnail,
# or 1|16 ft. This took on the general
# meaning of 1|16 and settled on the
# nail of a yard or 1|16 yards as its
# final value. [12]
UKpole 16.5 UKft # This was 15 Saxon feet, the Saxon
rope 20 UKft # foot (aka northern foot) being longer
englishell 45 UKinch
flemishell 27 UKinch
ell englishell # supposed to be measure from elbow to
# fingertips
span 9 UKinch # supposed to be distance from thumb
# to pinky with full hand extension
goad 4.5 UKft # used for cloth, possibly named after the
# stick used for prodding animals.
# misc obscure British units
hide 120 acre # English unit of land area dating to the 7th
# century, originally the amount of land
# that a single plowman could cultivate,
# which varied from 60-180 acres regionally.
# Standardized at Normon conquest.
virgate 1|4 hide
nook 1|2 virgate
rood furlong rod # Area of a strip a rod by a furlong
englishcarat troyounce/151.5 # Originally intended to be 4 grain
# but this value ended up being
# used in the London diamond market
mancus 2 oz
mast 2.5 lb
nailkeg 100 lbs
basebox 31360 in^2 # Used in metal plating
# alternate spellings
gramme gram
litre liter
dioptre diopter
sulphur sulfur
#
# Units derived the human body (may not be very accurate)
#
geometricpace 5 ft # distance between points where the same
# foot hits the ground
pace 2.5 ft # distance between points where alternate
# feet touch the ground
USmilitarypace 30 in # United States official military pace
USdoubletimepace 36 in # United States official doubletime pace
fingerbreadth 7|8 in # The finger is defined as either the width
fingerlength 4.5 in # or length of the finger
finger fingerbreadth
palmwidth hand # The palm is a unit defined as either the width
palmlength 8 in # or the length of the hand
hand 4 inch # width of hand
shaftment 6 inch # Distance from tip of outstretched thumb to the
# opposite side of the palm of the hand. The
# ending -ment is from the old English word
# for hand. [18]
smoot 5 ft + 7 in # Created as part of an MIT fraternity prank.
# In 1958 Oliver Smoot was used to measure
# the length of the Harvard Bridge, which was
# marked off in Smoot lengths. These
# markings have been maintained on the bridge
# since then and repainted by subsequent
# incoming fraternity members. During a
# bridge renovation the new sidewalk was
# scored every Smoot rather than at the
# customary 6 ft spacing.
tomcruise 5 ft + 7.75 in # Height of Tom Cruise
#
# Cooking measures
#
# Common abbreviations
tbl tablespoon
tbsp tablespoon
tblsp tablespoon
Tb tablespoon
tsp teaspoon
saltspoon 1|4 tsp
# US measures
uscup 8 usfloz
ustablespoon 1|16 uscup
usteaspoon 1|3 ustablespoon
ustbl ustablespoon
ustbsp ustablespoon
ustblsp ustablespoon
ustsp usteaspoon
metriccup 250 ml
stickbutter 1|4 lb # Butter in the USA is sold in one
# pound packages that contain four
# individually wrapped pieces. The
# pieces are marked into tablespoons,
# making it possible to measure out
# butter by volume by slicing the
# butter.
legalcup 240 ml # The cup used on nutrition labeling
legaltablespoon 1|16 legalcup
legaltbsp legaltablespoon
# Scoop size. Ice cream scoops in the US are marked with numbers
# indicating the number of scoops required to fill a US quart.
scoop(n) units=[1;cup] domain=[4,100] range=[0.04,1] \
32 usfloz / n ; 32 usfloz / scoop
# US can sizes.
number1can 10 usfloz
number2can 19 usfloz
number2.5can 3.5 uscups
number3can 4 uscups
number5can 7 uscups
number10can 105 usfloz
# British measures
brcup 1|2 brpint
brteacup 1|3 brpint
brtablespoon 15 ml # Also 5|8 brfloz, approx 17.7 ml
brteaspoon 1|3 brtablespoon # Also 1|4 brtablespoon
brdessertspoon 2 brteaspoon
dessertspoon brdessertspoon
dsp dessertspoon
brtsp brteaspoon
brtbl brtablespoon
brtbsp brtablespoon
brtblsp brtablespoon
# Australian
australiatablespoon 20 ml
austbl australiatablespoon
austbsp australiatablespoon
austblsp australiatablespoon
australiateaspoon 1|4 australiatablespoon
austsp australiateaspoon
# Italian
etto 100 g # Used for buying items like meat and
etti etto # cheese.
# Chinese
catty 0.5 kg
oldcatty 4|3 lbs # Before metric conversion.
tael 1|16 oldcatty # Should the tael be defined both ways?
mace 0.1 tael
oldpicul 100 oldcatty
picul 100 catty # Chinese usage
# Indian
seer 14400 grain # British Colonial standard
ser seer
maund 40 seer
pakistanseer 1 kg
pakistanmaund 40 pakistanseer
chittak 1|16 seer
tola 1|5 chittak
ollock 1|4 liter # Is this right?
# Japanese
japancup 200 ml
# densities of cooking ingredients from The Cake Bible by Rose Levy Beranbaum
# so you can convert '2 cups sugar' to grams, for example, or in the other
# direction grams could be converted to 'cup flour_scooped'.
butter 8 oz/uscup
butter_clarified 6.8 oz/uscup
cocoa_butter 9 oz/uscup
shortening 6.75 oz/uscup # vegetable shortening
oil 7.5 oz/uscup
cakeflour_sifted 3.5 oz/uscup # The density of flour depends on the
cakeflour_spooned 4 oz/uscup # measuring method. "Scooped", or
cakeflour_scooped 4.5 oz/uscup # "dip and sweep" refers to dipping a
flour_sifted 4 oz/uscup # measure into a bin, and then sweeping
flour_spooned 4.25 oz/uscup # the excess off the top. "Spooned"
flour_scooped 5 oz/uscup # means to lightly spoon into a measure
breadflour_sifted 4.25 oz/uscup # and then sweep the top. Sifted means
breadflour_spooned 4.5 oz/uscup # sifting the flour directly into a
breadflour_scooped 5.5 oz/uscup # measure and then sweeping the top.
cornstarch 120 grams/uscup
dutchcocoa_sifted 75 g/uscup # These are for Dutch processed cocoa
dutchcocoa_spooned 92 g/uscup
dutchcocoa_scooped 95 g/uscup
cocoa_sifted 75 g/uscup # These are for nonalkalized cocoa
cocoa_spooned 82 g/uscup
cocoa_scooped 95 g/uscup
heavycream 232 g/uscup
milk 242 g/uscup
sourcream 242 g/uscup
molasses 11.25 oz/uscup
cornsyrup 11.5 oz/uscup
honey 11.75 oz/uscup
sugar 200 g/uscup
powdered_sugar 4 oz/uscup
brownsugar_light 217 g/uscup # packed
brownsugar_dark 239 g/uscup
baking_powder 4.6 grams / ustsp
salt 6 g / ustsp
koshersalt 2.8 g / ustsp # Diamond Crystal kosher salt
koshersalt_morton 4.8 g / ustsp # Morton kosher salt
# Values are from the nutrition info
# on the packages
# Egg weights and volumes for a USA large egg
egg 50 grams # without shell
eggwhite 30 grams
eggyolk 18.6 grams
eggvolume 3 ustablespoons + 1|2 ustsp
eggwhitevolume 2 ustablespoons
eggyolkvolume 3.5 ustsp
# Alcohol density
ethanoldensity 0.7893 g/cm^3 # From CRC Handbook, 91st Edition
alcoholdensity ethanoldensity
#
# Density measures. Density has traditionally been measured on a variety of
# bizarre nonlinear scales.
#
# Density of a sugar syrup is frequently measured in candy making procedures.
# In the USA the boiling point of the syrup is measured. Some recipes instead
# specify the density using degrees Baume. Conversion between degrees Baume
# and the boiling point measure has proved elusive. This table appeared in one
# text, and provides a fragmentary relationship to the concentration.
#
# temp(C) conc (%)
# 100 30
# 101 40
# 102 50
# 103 60
# 106 70
# 112 80
# 123 90
# 140 95
# 151 97
# 160 98.2
# 166 99.5
# 171 99.6
#
# The best source identified to date came from "Boiling point elevation of
# technical sugarcane solutions and its use in automatic pan boiling" by
# Michael Saska. International Sugar Journal, 2002, 104, 1247, pp 500-507.
#
# But I'm using equation (3) which is credited to Starzak and Peacock,
# "Water activity coefficient in aqueous solutions of sucrose--A comprehensive
# data analysis. Zuckerindustrie, 122, 380-387. (I couldn't find this
# document.)
#
# Note that the range of validity is uncertain, but answers are in agreement
# with the above table all the way to 99.6.
#
# The original equation has a parameter for the boiling point of water, which
# of course varies with altitude. It also includes various other model
# parameters. The input is the molar concentration of sucrose in the solution,
# (moles sucrose) / (total moles).
#
# Bsp 3797.06 degC
# Csp 226.28 degC
# QQ -17638 J/mol
# asp -1.0038
# bsp -0.24653
# tbw 100 degC # boiling point of water
# sugar_bpe_orig(x) ((1-QQ/R Bsp * x^2 (1+asp x + bsp x^2) (tbw + Csp) \
# /(tbw+stdtemp)) / (1+(tbw + Csp)/Bsp *ln(1-x))-1) * (tbw + Csp)
#
# To convert mass concentration (brix) to molar concentration
#
# sc(x) (x / 342.3) / (( x/342.3) + (100-x)/18.02); \
# 100 sc 342.3|18.02 / (sc (342.3|18.02-1)+1)
#
# Here is a simplified version of this equation where the temperature of boiling
# water has been fixed at 100 degrees Celsius and the argument is now the
# concentration (brix).
#
# sugar_bpe(x) ((1+ 0.48851085 * sc(x)^2 (1+ -1.0038 sc(x) + -0.24653 sc(x)^2)) \
# / (1+0.08592964 ln(1-sc(x)))-1) 326.28 K
#
#
# The formula is not invertible, so to implement it in units we unfortunately
# must turn it into a table.
# This table gives the boiling point elevation as a function of the sugar syrup
# concentration expressed as a percentage.
sugar_conc_bpe[K] \
0 0.0000 5 0.0788 10 0.1690 15 0.2729 20 0.3936 25 0.5351 \
30 0.7027 35 0.9036 40 1.1475 42 1.2599 44 1.3825 46 1.5165 \
48 1.6634 50 1.8249 52 2.0031 54 2.2005 56 2.4200 58 2.6651 \
60 2.9400 61 3.0902 62 3.2499 63 3.4198 64 3.6010 65 3.7944 \
66 4.0012 67 4.2227 68 4.4603 69 4.7156 70 4.9905 71 5.2870 \
72 5.6075 73 5.9546 74 6.3316 75 6.7417 76 7.1892 77 7.6786 \
78.0 8.2155 79.0 8.8061 80.0 9.4578 80.5 9.8092 81.0 10.1793 \
81.5 10.5693 82.0 10.9807 82.5 11.4152 83.0 11.8743 83.5 12.3601 \
84.0 12.8744 84.5 13.4197 85.0 13.9982 85.5 14.6128 86.0 15.2663 \
86.5 15.9620 87.0 16.7033 87.5 17.4943 88.0 18.3391 88.5 19.2424 \
89.0 20.2092 89.5 21.2452 90.0 22.3564 90.5 23.5493 91.0 24.8309 \
91.5 26.2086 92.0 27.6903 92.5 29.2839 93.0 30.9972 93.5 32.8374 \
94.0 34.8104 94.5 36.9195 95.0 39.1636 95.5 41.5348 96.0 44.0142 \
96.5 46.5668 97.0 49.1350 97.5 51.6347 98.0 53.9681 98.1 54.4091 \
98.2 54.8423 98.3 55.2692 98.4 55.6928 98.5 56.1174 98.6 56.5497 \
98.7 56.9999 98.8 57.4828 98.9 58.0206 99.0 58.6455 99.1 59.4062 \
99.2 60.3763 99.3 61.6706 99.4 63.4751 99.5 66.1062 99.6 70.1448 \
99.7 76.7867
# Using the brix table we can use this to produce a mapping from boiling point
# to density which makes all of the units interconvertible. Because the brix
# table stops at 95 this approach works up to a boiling point elevation of 39 K
# or a boiling point of 139 C / 282 F, which is the "soft crack" stage in candy
# making. The "hard crack" stage continues up to 310 F.
# Boiling point elevation
sugar_bpe(T) units=[K;g/cm^3] domain=[0,39.1636] range=[0.99717,1.5144619] \
brix(~sugar_conc_bpe(T)); sugar_conc_bpe(~brix(sugar_bpe))
# Absolute boiling point (produces an absolute temperature)
sugar_bp(T) units=[K;g/cm^3] domain=[373.15,412.3136] \
range=[0.99717,1.5144619] \
brix(~sugar_conc_bpe(T-tempC(100))) ;\
sugar_conc_bpe(~brix(sugar_bp))+tempC(100)
# In practice dealing with the absolute temperature is annoying because it is
# not possible to convert to a nested function, so you're stuck retyping the
# absolute temperature in Kelvins to convert to celsius or Fahrenheit. To
# prevent this we supply definitions that build in the temperature conversion
# and produce results in the Fahrenheit and Celsius scales. So using these
# measures, to convert 46 degrees Baume to a Fahrenheit boiling point:
#
# You have: baume(45)
# You want: sugar_bpF
# 239.05647
#
sugar_bpF(T) units=[1;g/cm^3] domain=[212,282.49448] range=[0.99717,1.5144619]\
brix(~sugar_conc_bpe(tempF(T)+-tempC(100))) ;\
~tempF(sugar_conc_bpe(~brix(sugar_bpF))+tempC(100))
sugar_bpC(T) units=[1;g/cm^3] domain=[100,139.1636] range=[0.99717,1.5144619]\
brix(~sugar_conc_bpe(tempC(T)+-tempC(100))) ;\
~tempC(sugar_conc_bpe(~brix(sugar_bpC))+tempC(100))
# Degrees Baume is used in European recipes to specify the density of a sugar
# syrup. An entirely different definition is used for densities below
# 1 g/cm^3. An arbitrary constant appears in the definition. This value is
# equal to 145 in the US, but was according to [], the old scale used in
# Holland had a value of 144, and the new scale or Gerlach scale used 146.78.
baumeconst 145 # US value
baume(d) units=[1;g/cm^3] domain=[0,145) range=[1,) \
(baumeconst/(baumeconst+-d)) g/cm^3 ; \
(baume+((-g)/cm^3)) baumeconst / baume
# It's not clear if this value was ever used with negative degrees.
twaddell(x) units=[1;g/cm^3] domain=[-200,) range=[0,) \
(1 + 0.005 x) g / cm^3 ; \
200 (twaddell / (g/cm^3) +- 1)
# The degree quevenne is a unit for measuring the density of milk.
# Similarly it's unclear if negative values were allowed here.
quevenne(x) units=[1;g/cm^3] domain=[-1000,) range=[0,) \
(1 + 0.001 x) g / cm^3 ; \
1000 (quevenne / (g/cm^3) +- 1)
# Degrees brix measures sugar concentration by weigh as a percentage, so a
# solution that is 3 degrees brix is 3% sugar by weight. This unit was named
# after Adolf Brix who invented a hydrometer that read this percentage
# directly. This data is from Table 114 of NIST Circular 440, "Polarimetry,
# Saccharimetry and the Sugars". It gives apparent specific gravity at 20
# degrees Celsius of various sugar concentrations. As rendered below this
# data is converted to apparent density at 20 degrees Celsius using the
# density figure for water given in the same NIST reference. They use the
# word "apparent" to refer to measurements being made in air with brass
# weights rather than vacuum.
brix[0.99717g/cm^3]\
0 1.00000 1 1.00390 2 1.00780 3 1.01173 4 1.01569 5 1.01968 \
6 1.02369 7 1.02773 8 1.03180 9 1.03590 10 1.04003 11 1.04418 \
12 1.04837 13 1.05259 14 1.05683 15 1.06111 16 1.06542 17 1.06976 \
18 1.07413 19 1.07853 20 1.08297 21 1.08744 22 1.09194 23 1.09647 \
24 1.10104 25 1.10564 26 1.11027 27 1.11493 28 1.11963 29 1.12436 \
30 1.12913 31 1.13394 32 1.13877 33 1.14364 34 1.14855 35 1.15350 \
36 1.15847 37 1.16349 38 1.16853 39 1.17362 40 1.17874 41 1.18390 \
42 1.18910 43 1.19434 44 1.19961 45 1.20491 46 1.21026 47 1.21564 \
48 1.22106 49 1.22652 50 1.23202 51 1.23756 52 1.24313 53 1.24874 \
54 1.25439 55 1.26007 56 1.26580 57 1.27156 58 1.27736 59 1.28320 \
60 1.28909 61 1.29498 62 1.30093 63 1.30694 64 1.31297 65 1.31905 \
66 1.32516 67 1.33129 68 1.33748 69 1.34371 70 1.34997 71 1.35627 \
72 1.36261 73 1.36900 74 1.37541 75 1.38187 76 1.38835 77 1.39489 \
78 1.40146 79 1.40806 80 1.41471 81 1.42138 82 1.42810 83 1.43486 \
84 1.44165 85 1.44848 86 1.45535 87 1.46225 88 1.46919 89 1.47616 \
90 1.48317 91 1.49022 92 1.49730 93 1.50442 94 1.51157 95 1.51876
# Density measure invented by the American Petroleum Institute. Lighter
# petroleum products are more valuable, and they get a higher API degree.
#
# The intervals of range and domain should be open rather than closed.
#
apidegree(x) units=[1;g/cm^3] domain=[-131.5,) range=[0,) \
141.5 g/cm^3 / (x+131.5) ; \
141.5 (g/cm^3) / apidegree + (-131.5)
#
# Average densities of various woods (dried)
# Data from The Wood Database https://www.wood-database.com
#
# North American Hardwoods
wood_cherry 35 lb/ft^3
wood_redoak 44 lb/ft^3
wood_whiteoak 47 lb/ft^3
wood_blackwalnut 38 lb/ft^3
wood_walnut wood_blackwalnut
wood_birch 43 lb/ft^3
wood_hardmaple 44 lb/ft^3
wood_bigleafmaple 34 lb/ft^3
wood_boxeldermaple 30 lb/ft^3
wood_redmaple 38 lb/ft^3
wood_silvermaple 33 lb/ft^3
wood_stripedmaple 32 lb/ft^3
wood_softmaple (wood_bigleafmaple \
+ wood_boxeldermaple \
+ wood_redmaple \
+ wood_silvermaple \
+ wood_stripedmaple) / 5
wood_poplar 29 lb/ft^3
wood_beech 45 lb/ft^3
# North American Softwoods
wood_jeffreypine 28 lb/ft^3
wood_ocotepine 44 lb/ft^3
wood_ponderosapine 28 lb/ft^3
wood_loblollypine 35 lb/ft^3
wood_longleafpine 41 lb/ft^3
wood_shortleafpine 35 lb/ft^3
wood_slashpine 41 lb/ft^3
wood_yellowpine (wood_loblollypine \
+ wood_longleafpine \
+ wood_shortleafpine \
+ wood_slashpine) / 4
wood_redpine 34 lb/ft^3
wood_easternwhitepine 25 lb/ft^3
wood_westernwhitepine 27 lb/ft^3
wood_whitepine (wood_easternwhitepine + wood_westernwhitepine) / 2
wood_douglasfir 32 lb/ft^3
wood_blackspruce 28 lb/ft^3
wood_engelmannspruce 24 lb/ft^3
wood_redspruce 27 lb/ft^3
wood_sitkaspruce 27 lb/ft^3
wood_whitespruce 27 lb/ft^3
wood_spruce (wood_blackspruce \
+ wood_engelmannspruce \
+ wood_redspruce \
+ wood_sitkaspruce \
+ wood_whitespruce) / 5
# Other woods
wood_basswood 26 lb/ft^3
wood_balsa 9 lb/ft^3
wood_ebony_gaboon 60 lb/ft^3
wood_ebony_macassar 70 lb/ft^3
wood_mahogany 37 lb/ft^3 # True (Honduran) mahogany,
# Swietenia macrophylla
wood_teak 41 lb/ft^3
wood_rosewood_brazilian 52 lb/ft^3
wood_rosewood_honduran 64 lb/ft^3
wood_rosewood_indian 52 lb/ft^3
wood_cocobolo 69 lb/ft^3
wood_bubinga 56 lb/ft^3
wood_zebrawood 50 lb/ft^3
wood_koa 38 lb/ft^3
wood_snakewood 75.7 lb/ft^3
wood_lignumvitae 78.5 lb/ft^3
wood_blackwood 79.3 lb/ft^3
wood_blackironwood 84.5 lb/ft^3 # Krugiodendron ferreum, listed
# in database as the heaviest wood
#
# Modulus of elasticity of selected woods.
# Data from The Wood Database https://www.wood-database.com
#
# North American Hardwoods
wood_mod_beech 1.720e6 lbf/in^2
wood_mod_birchyellow 2.010e6 lbf/in^2
wood_mod_birch wood_mod_birchyellow
wood_mod_cherry 1.490e6 lbf/in^2
wood_mod_hardmaple 1.830e6 lbf/in^2
wood_mod_bigleafmaple 1.450e6 lbf/in^2
wood_mod_boxeldermaple 1.050e6 lbf/in^2
wood_mod_redmaple 1.640e6 lbf/in^2
wood_mod_silvermaple 1.140e6 lbf/in^2
wood_mod_softmaple (wood_mod_bigleafmaple \
+ wood_mod_boxeldermaple \
+ wood_mod_redmaple \
+ wood_mod_silvermaple) / 4
wood_mod_redoak 1.761e6 lbf/in^2
wood_mod_whiteoak 1.762e6 lbf/in^2
wood_mod_poplar 1.580e6 lbf/in^2
wood_mod_blackwalnut 1.680e6 lbf/in^2
wood_mod_walnut wood_mod_blackwalnut
# North American Softwoods
wood_mod_jeffreypine 1.240e6 lbf/in^2
wood_mod_ocotepine 2.209e6 lbf/in^2
wood_mod_ponderosapine 1.290e6 lbf/in^2
wood_mod_loblollypine 1.790e6 lbf/in^2
wood_mod_longleafpine 1.980e6 lbf/in^2
wood_mod_shortleafpine 1.750e6 lbf/in^2
wood_mod_slashpine 1.980e6 lbf/in^2
wood_mod_yellowpine (wood_mod_loblollypine \
+ wood_mod_longleafpine \
+ wood_mod_shortleafpine \
+ wood_mod_slashpine) / 4
wood_mod_redpine 1.630e6 lbf/in^2
wood_mod_easternwhitepine 1.240e6 lbf/in^2
wood_mod_westernwhitepine 1.460e6 lbf/in^2
wood_mod_whitepine (wood_mod_easternwhitepine + \
wood_mod_westernwhitepine) / 2
wood_mod_douglasfir 1.765e6 lbf/in^2
wood_mod_blackspruce 1.523e6 lbf/in^2
wood_mod_englemannspruce 1.369e6 lbf/in^2
wood_mod_redspruce 1.560e6 lbf/in^2
wood_mod_sitkaspruce 1.600e6 lbf/in^2
wood_mod_whitespruce 1.315e6 lbf/in^2
wood_mod_spruce (wood_mod_blackspruce \
+ wood_mod_englemannspruce \
+ wood_mod_redspruce + wood_mod_sitkaspruce \
+ wood_mod_whitespruce) / 5
# Other woods
wood_mod_balsa 0.538e6 lbf/in^2
wood_mod_basswood 1.460e6 lbf/in^2
wood_mod_blackwood 2.603e6 lbf/in^2 # African, Dalbergia melanoxylon
wood_mod_bubinga 2.670e6 lbf/in^2
wood_mod_cocobolo 2.712e6 lbf/in^2
wood_mod_ebony_gaboon 2.449e6 lbf/in^2
wood_mod_ebony_macassar 2.515e6 lbf/in^2
wood_mod_blackironwood 2.966e6 lbf/in^2 # Krugiodendron ferreum
wood_mod_koa 1.503e6 lbf/in^2
wood_mod_lignumvitae 2.043e6 lbf/in^2
wood_mod_mahogany 1.458e6 lbf/in^2 # True (Honduran) mahogany,
# Swietenia macrophylla
wood_mod_rosewood_brazilian 2.020e6 lbf/in^2
wood_mod_rosewood_honduran 3.190e6 lbf/in^2
wood_mod_rosewood_indian 1.668e6 lbf/in^2
wood_mod_snakewood 3.364e6 lbf/in^2
wood_mod_teak 1.781e6 lbf/in^2
wood_mod_zebrawood 2.374e6 lbf/in^2
#
# Area of countries and other regions. This is the "total area" which
# includes land and water areas within international boundaries and
# coastlines. Data from January, 2019.
#
# except as noted, sources are
# https://en.wikipedia.org/wiki/List_of_countries_and_dependencies_by_area
# US Central Intelligence Agency: The World Factbook
# https://www.cia.gov/the-world-factbook/
area_russia 17098246 km^2
area_antarctica 14000000 km^2
# area_canada is covered below as sum of province and territory areas
area_china 9596961 km^2
# area_unitedstates is covered below as sum of state areas
# includes only the 50 states and District of Columbia
area_us area_unitedstates
area_brazil 8515767 km^2
area_australia 7692024 km^2
# area_europeanunion is covered below as sum of member areas
area_india 3287263 km^2
area_argentina 2780400 km^2
area_kazakhstan 2724900 km^2
area_algeria 2381741 km^2
area_drcongo 2344858 km^2
area_greenland 2166086 km^2
area_saudiarabia 2149690 km^2
area_mexico 1964375 km^2
area_indonesia 1910931 km^2
area_sudan 1861484 km^2
area_libya 1759540 km^2
area_iran 1648195 km^2
area_mongolia 1564110 km^2
area_peru 1285216 km^2
area_chad 1284000 km^2
area_niger 1267000 km^2
area_angola 1246700 km^2
area_mali 1240192 km^2
area_southafrica 1221037 km^2
area_colombia 1141748 km^2
area_ethiopia 1104300 km^2
area_bolivia 1098581 km^2
area_mauritania 1030700 km^2
area_egypt 1002450 km^2
area_tanzania 945087 km^2
area_nigeria 923768 km^2
area_venezuela 916445 km^2
area_pakistan 881912 km^2
area_namibia 825615 km^2
area_mozambique 801590 km^2
area_turkey 783562 km^2
area_chile 756102 km^2
area_zambia 752612 km^2
area_myanmar 676578 km^2
area_burma area_myanmar
area_afghanistan 652230 km^2
area_southsudan 644329 km^2
area_france 640679 km^2
area_somalia 637657 km^2
area_centralafrica 622984 km^2
area_ukraine 603500 km^2
area_crimea 27000 km^2 # occupied by Russia; included in
# (Encyclopedia Britannica)
area_madagascar 587041 km^2
area_botswana 581730 km^2
area_kenya 580367 km^2
area_yemen 527968 km^2
area_thailand 513120 km^2
area_spain 505992 km^2
area_turkmenistan 488100 km^2
area_cameroon 475422 km^2
area_papuanewguinea 462840 km^2
area_sweden 450295 km^2
area_uzbekistan 447400 km^2
area_morocco 446550 km^2
area_iraq 438317 km^2
area_paraguay 406752 km^2
area_zimbabwe 390757 km^2
area_japan 377973 km^2
area_germany 357114 km^2
area_congorepublic 342000 km^2
area_finland 338424 km^2
area_vietnam 331212 km^2
area_malaysia 330803 km^2
area_norway 323802 km^2
area_ivorycoast 322463 km^2
area_poland 312696 km^2
area_oman 309500 km^2
area_italy 301339 km^2
area_philippines 300000 km^2
area_ecuador 276841 km^2
area_burkinafaso 274222 km^2
area_newzealand 270467 km^2
area_gabon 267668 km^2
area_westernsahara 266000 km^2
area_guinea 245857 km^2
# area_unitedkingdom is covered below
area_uganda 241550 km^2
area_ghana 238533 km^2
area_romania 238397 km^2
area_laos 236800 km^2
area_guyana 214969 km^2
area_belarus 207600 km^2
area_kyrgyzstan 199951 km^2
area_senegal 196722 km^2
area_syria 185180 km^2
area_golanheights 1150 km^2 # occupied by Israel; included in
# Syria (Encyclopedia Britannica)
area_cambodia 181035 km^2
area_uruguay 176215 km^2
area_somaliland 176120 km^2
area_suriname 163820 km^2
area_tunisia 163610 km^2
area_bangladesh 147570 km^2
area_nepal 147181 km^2
area_tajikistan 143100 km^2
area_greece 131990 km^2
area_nicaragua 130373 km^2
area_northkorea 120540 km^2
area_malawi 118484 km^2
area_eritrea 117600 km^2
area_benin 114763 km^2
area_honduras 112492 km^2
area_liberia 111369 km^2
area_bulgaria 110879 km^2
area_cuba 109884 km^2
area_guatemala 108889 km^2
area_iceland 103000 km^2
area_southkorea 100210 km^2
area_hungary 93028 km^2
area_portugal 92090 km^2
area_jordan 89342 km^2
area_serbia 88361 km^2
area_azerbaijan 86600 km^2
area_austria 83871 km^2
area_uae 83600 km^2
area_czechia 78865 km^2
area_czechrepublic area_czechia
area_panama 75417 km^2
area_sierraleone 71740 km^2
area_ireland 70273 km^2
area_georgia 69700 km^2
area_srilanka 65610 km^2
area_lithuania 65300 km^2
area_latvia 64559 km^2
area_togo 56785 km^2
area_croatia 56594 km^2
area_bosnia 51209 km^2
area_costarica 51100 km^2
area_slovakia 49037 km^2
area_dominicanrepublic 48671 km^2
area_estonia 45227 km^2
area_denmark 43094 km^2
area_netherlands 41850 km^2
area_switzerland 41284 km^2
area_bhutan 38394 km^2
area_taiwan 36193 km^2
area_guineabissau 36125 km^2
area_moldova 33846 km^2
area_belgium 30528 km^2
area_lesotho 30355 km^2
area_armenia 29743 km^2
area_solomonislands 28896 km^2
area_albania 28748 km^2
area_equitorialguinea 28051 km^2
area_burundi 27834 km^2
area_haiti 27750 km^2
area_rwanda 26338 km^2
area_northmacedonia 25713 km^2
area_djibouti 23200 km^2
area_belize 22966 km^2
area_elsalvador 21041 km^2
area_israel 20770 km^2
area_slovenia 20273 km^2
area_fiji 18272 km^2
area_kuwait 17818 km^2
area_eswatini 17364 km^2
area_easttimor 14919 km^2
area_bahamas 13943 km^2
area_montenegro 13812 km^2
area_vanatu 12189 km^2
area_qatar 11586 km^2
area_gambia 11295 km^2
area_jamaica 10991 km^2
area_kosovo 10887 km^2
area_lebanon 10452 km^2
area_cyprus 9251 km^2
area_puertorico 9104 km^2 # United States territory; not included
# in United States area
area_westbank 5860 km^2 # (CIA World Factbook)
area_hongkong 2755 km^2
area_luxembourg 2586 km^2
area_singapore 716 km^2
area_gazastrip 360 km^2 # (CIA World Factbook)
area_malta 316 km^2 # smallest EU country
area_liechtenstein 160 km^2
area_monaco 2.02 km^2
area_vaticancity 0.44 km^2
# Members as of 1 Feb 2020
area_europeanunion area_austria + area_belgium + area_bulgaria \
+ area_croatia + area_cyprus + area_czechia + area_denmark \
+ area_estonia + area_finland + area_france + area_germany \
+ area_greece + area_hungary + area_ireland + area_italy \
+ area_latvia + area_lithuania + area_luxembourg \
+ area_malta + area_netherlands + area_poland \
+ area_portugal + area_romania + area_slovakia \
+ area_slovenia + area_spain + area_sweden
area_eu area_europeanunion
#
# Areas of the individual US states
#
# https://en.wikipedia.org/wiki/List_of_U.S._states_and_territories_by_area
#
# United States Summary: 2010, Population and Housing Unit Counts, Table 18, p. 41
# Issued September 2012
area_alaska 1723336.8 km^2
area_texas 695661.6 km^2
area_california 423967.4 km^2
area_montana 380831.1 km^2
area_newmexico 314917.4 km^2
area_arizona 295233.5 km^2
area_nevada 286379.7 km^2
area_colorado 269601.4 km^2
area_oregon 254799.2 km^2
area_wyoming 253334.5 km^2
area_michigan 250486.8 km^2
area_minnesota 225162.8 km^2
area_utah 219881.9 km^2
area_idaho 216442.6 km^2
area_kansas 213100.0 km^2
area_nebraska 200329.9 km^2
area_southdakota 199728.7 km^2
area_washington 184660.8 km^2
area_northdakota 183107.8 km^2
area_oklahoma 181037.2 km^2
area_missouri 180540.3 km^2
area_florida 170311.7 km^2
area_wisconsin 169634.8 km^2
area_georgia_us 153910.4 km^2
area_illinois 149995.4 km^2
area_iowa 145745.9 km^2
area_newyork 141296.7 km^2
area_northcarolina 139391.0 km^2
area_arkansas 137731.8 km^2
area_alabama 135767.4 km^2
area_louisiana 135658.7 km^2
area_mississippi 125437.7 km^2
area_pennsylvania 119280.2 km^2
area_ohio 116097.7 km^2
area_virginia 110786.6 km^2
area_tennessee 109153.1 km^2
area_kentucky 104655.7 km^2
area_indiana 94326.2 km^2
area_maine 91633.1 km^2
area_southcarolina 82932.7 km^2
area_westvirginia 62755.5 km^2
area_maryland 32131.2 km^2
area_hawaii 28313.0 km^2
area_massachusetts 27335.7 km^2
area_vermont 24906.3 km^2
area_newhampshire 24214.2 km^2
area_newjersey 22591.4 km^2
area_connecticut 14357.4 km^2
area_delaware 6445.8 km^2
area_rhodeisland 4001.2 km^2
area_districtofcolumbia 177.0 km^2
area_unitedstates area_alabama + area_alaska + area_arizona \
+ area_arkansas + area_california + area_colorado \
+ area_connecticut + area_delaware \
+ area_districtofcolumbia + area_florida \
+ area_georgia_us + area_hawaii + area_idaho \
+ area_illinois + area_indiana + area_iowa \
+ area_kansas + area_kentucky + area_louisiana \
+ area_maine + area_maryland + area_massachusetts \
+ area_michigan + area_minnesota + area_mississippi \
+ area_missouri + area_montana + area_nebraska \
+ area_nevada + area_newhampshire + area_newjersey \
+ area_newmexico + area_newyork + area_northcarolina \
+ area_northdakota + area_ohio + area_oklahoma \
+ area_oregon + area_pennsylvania + area_rhodeisland \
+ area_southcarolina + area_southdakota \
+ area_tennessee + area_texas + area_utah \
+ area_vermont + area_virginia + area_washington \
+ area_westvirginia + area_wisconsin + area_wyoming
# Total area of Canadian province and territories
#
# Statistics Canada, "Land and freshwater area, by province and territory",
# 2016-10-07:
#
# https://www150.statcan.gc.ca/n1/pub/11-402-x/2012000/chap/geo/tbl/tbl06-eng.htm
area_ontario 1076395 km^2 # confederated 1867-Jul-01
area_quebec 1542056 km^2 # confederated 1867-Jul-01
area_novascotia 55284 km^2 # confederated 1867-Jul-01
area_newbrunswick 72908 km^2 # confederated 1867-Jul-01
area_canada_original area_ontario + area_quebec + area_novascotia \
+ area_newbrunswick
area_manitoba 647797 km^2 # confederated 1870-Jul-15
area_britishcolumbia 944735 km^2 # confederated 1871-Jul-20
area_princeedwardisland 5660 km^2 # confederated 1873-Jul-01
area_canada_additional area_manitoba + area_britishcolumbia \
+ area_princeedwardisland
area_alberta 661848 km^2 # confederated 1905-Sep-01
area_saskatchewan 651036 km^2 # confederated 1905-Sep-01
area_newfoundlandandlabrador 405212 km^2 # confederated 1949-Mar-31
area_canada_recent area_alberta + area_saskatchewan \
+ area_newfoundlandandlabrador
area_canada_provinces area_canada_original + area_canada_additional \
+ area_canada_recent
area_northwestterritories 1346106 km^2 # NT confederated 1870-Jul-15
area_yukon 482443 km^2 # YT confederated 1898-Jun-13
area_nunavut 2093190 km^2 # NU confederated 1999-Apr-01
area_canada_territories area_northwestterritories + area_yukon \
+ area_nunavut
area_canada area_canada_provinces + area_canada_territories
# area-uk-countries.units - UK country (/province) total areas
# https://en.wikipedia.org/wiki/Countries_of_the_United_Kingdom#Statistics
# GB is official UK country code for some purposes but internally is a Kingdom
#
# areas from A Beginners Guide to UK Geography 2019 v1.0, Office for National Statistics
# England: country; 0927-Jul-12 united; 1603-Mar-24 union of crowns
area_england 132947.76 km^2
#
# Wales: 1282 conquered; 1535 union; principality until 2011
area_wales 21224.48 km^2
#
# England and Wales: nation; 1535 union
area_englandwales area_england + area_wales
#
# Scotland: country; ~900 united; 1603-Mar-24 union of crowns
area_scotland 80226.36 km^2
#
# Great Britain: kingdom; excludes NI;
# 1707 Treaty and Acts of Union: union of parliaments
area_greatbritain area_england + area_wales + area_scotland
area_gb area_greatbritain
#
# Northern Ireland: province; Ireland: 1177 Henry II lordship;
# 1542 Henry VIII kingdom; 1652 Cromwell commonwealth;
# 1691 William III kingdom; 1800 Acts of Union: UK of GB & Ireland;
# 1921 Irish Free State independent of UK
area_northernireland 14133.38 km^2
#
# United Kingdom of GB & NI: 1800 Acts of Union: UK of GB & Ireland;
# 1921 Irish Free State independent of UK
area_unitedkingdom area_greatbritain + area_northernireland
area_uk area_unitedkingdom
#
# Units derived from imperial system
#
ouncedal oz ft / s^2 # force which accelerates an ounce
# at 1 ft/s^2
poundal lb ft / s^2 # same thing for a pound
tondal longton ft / s^2 # and for a ton
pdl poundal
osi ounce force / inch^2 # used in aviation
psi pound force / inch^2
psia psi # absolute pressure
# Note that gauge pressure can be given
# using the gaugepressure() and
# psig() nonlinear unit definitions
tsi ton force / inch^2
reyn psi sec
slug lbf s^2 / ft
slugf slug force
slinch lbf s^2 / inch # Mass unit derived from inch second
slinchf slinch force # pound-force system. Used in space
# applications where in/sec^2 was a
# natural acceleration measure.
geepound slug
lbf lb force
tonf ton force
lbm lb
kip 1000 lbf # from kilopound
ksi kip / in^2
mil 0.001 inch
thou 0.001 inch
tenth 0.0001 inch # one tenth of one thousandth of an inch
millionth 1e-6 inch # one millionth of an inch
circularinch 1|4 pi in^2 # area of a one-inch diameter circle
circleinch circularinch # A circle with diameter d inches has
# an area of d^2 circularinches
cylinderinch circleinch inch # Cylinder h inch tall, d inches diameter
# has volume d^2 h cylinder inches
circularmil 1|4 pi mil^2 # area of one-mil diameter circle
cmil circularmil
MCM kcmil # older initialism for thousand circular mills
cental 100 pound
centner cental
# Shotgun gauge measures the inside diameter of the barrel by counting
# the number of spherical lead balls you can make to fit that barrel
# using a pound of lead. Equivalently, this means that an n gauge gun
# has a bore diameter that fits a ball of lead that weighs 1|n pounds
shotgungauge(ga) units=[1;m] domain=(0,] range=(0,] \
2 ~spherevol(1 pound / ga leaddensity) ; \
1 pound / leaddensity spherevol(shotgungauge/2)
shotgunga() shotgungauge
caliber 0.01 inch # for measuring bullets
duty ft lbf
celo ft / s^2
jerk ft / s^3
australiapoint 0.01 inch # The "point" is used to measure rainfall
# in Australia
sabin ft^2 # Measure of sound absorption equal to the
# absorbing power of one square foot of
# a perfectly absorbing material. The
# sound absorptivity of an object is the
# area times a dimensionless
# absorptivity coefficient.
standardgauge 4 ft + 8.5 in # Standard width between railroad track
flag 5 ft^2 # Construction term referring to sidewalk.
rollwallpaper 30 ft^2 # Area of roll of wall paper
fillpower in^3 / ounce # Density of down at standard pressure.
# The best down has 750-800 fillpower.
pinlength 1|16 inch # A #17 pin is 17/16 in long in the USA.
buttonline 1|40 inch # The line was used in 19th century USA
# to measure width of buttons.
beespace 1|4 inch # Bees will fill any space that is smaller
# than the bee space and leave open
# spaces that are larger. The size of
# the space varies with species.
diamond 8|5 ft # Marking on US tape measures that is
# useful to carpenters who wish to place
# five studs in an 8 ft distance. Note
# that the numbers appear in red every
# 16 inches as well, giving six
# divisions in 8 feet.
retmaunit 1.75 in # Height of rack mountable equipment.
U retmaunit # Equipment should be 1|32 inch narrower
RU U # than its U measurement indicates to
# allow for clearance, so 4U=(6+31|32)in
# RETMA stands for the former name of
# the standardizing organization, Radio
# Electronics Television Manufacturers
# Association. This organization is now
# called the Electronic Industries
# Alliance (EIA) and the rack standard
# is specified in EIA RS-310-D.
count per pound # For measuring the size of shrimp
flightlevel 100 ft # Flight levels are used to ensure safe
FL flightlevel # vertical separation between aircraft
# despite variations in local air
# pressure. Flight levels define
# altitudes based on a standard air
# pressure so that altimeter calibration
# is not needed. This means that
# aircraft at separated flight levels
# are guaranteed to be separated.
# Hence the definition of 100 feet is
# a nominal, not true, measure.
# Customarily written with no space in
# the form FL290, which will not work in
# units. But note "FL 290" will work.
#
# Other units of work, energy, power, etc
#
# Calorie: approximate energy to raise a gram of water one degree celsius
calorie cal_th # Default is the thermochemical calorie
cal calorie
calorie_th 4.184 J # Thermochemical calorie, defined in 1930
thermcalorie calorie_th # by Frederick Rossini as 4.1833 J to
cal_th calorie_th # avoid difficulties associated with the
# uncertainty in the heat capacity of
# water. In 1948 the value of the joule
# was changed, so the thermochemical
# calorie was redefined to 4.184 J.
# This kept the energy measured by this
# unit the same.
calorie_IT 4.1868 J # International (Steam) Table calorie,
cal_IT calorie_IT # defined in 1929 as watt-hour/860 or
# equivalently 180|43 joules. At this
# time the international joule had a
# different value than the modern joule,
# and the values were different in the
# USA and in Europe. In 1956 at the
# Fifth International Conference on
# Properties of Steam the exact
# definition given here was adopted.
calorie_15 4.18580 J # Energy to go from 14.5 to 15.5 degC
cal_15 calorie_15
calorie_fifteen cal_15
calorie_20 4.18190 J # Energy to go from 19.5 to 20.5 degC
cal_20 calorie_20
calorie_twenty calorie_20
calorie_4 4.204 J # Energy to go from 3.5 to 4.5 degC
cal_4 calorie_4
calorie_four calorie_4
cal_mean 4.19002 J # 1|100 energy to go from 0 to 100 degC
Calorie kilocalorie # the food Calorie
thermie 1e6 cal_15 # Heat required to raise the
# temperature of a tonne of
# water from 14.5 to 15.5 degC.
# btu definitions: energy to raise a pound of water 1 degF
btu btu_IT # International Table BTU is the default
britishthermalunit btu
btu_IT cal_IT lb degF / gram K
btu_th cal_th lb degF / gram K
btu_mean cal_mean lb degF / gram K
btu_15 cal_15 lb degF / gram K
btu_ISO 1055.06 J # Exact, rounded ISO definition based
# on the IT calorie
quad quadrillion btu
ECtherm 1e5 btu_ISO # Exact definition
UStherm 1.054804e8 J # Exact definition
therm UStherm
# Water latent heat from [23]
water_fusion_heat 6.01 kJ/mol / (18.015 g/mol) # At 0 deg C
water_vaporization_heat 2256.4 J/g # At saturation, 100 deg C, 101.42 kPa
# Specific heat capacities of various substances
#
SPECIFIC_HEAT ENERGY / MASS / TEMPERATURE_DIFFERENCE
SPECIFIC_HEAT_CAPACITY ENERGY / MASS / TEMPERATURE_DIFFERENCE
specificheat_water calorie / g K
water_specificheat specificheat_water
# Values from www.engineeringtoolbox.com/specific-heat-metals-d_152.html
specificheat_aluminum 0.91 J/g K
specificheat_antimony 0.21 J/g K
specificheat_barium 0.20 J/g K
specificheat_beryllium 1.83 J/g K
specificheat_bismuth 0.13 J/g K
specificheat_cadmium 0.23 J/g K
specificheat_cesium 0.24 J/g K
specificheat_chromium 0.46 J/g K
specificheat_cobalt 0.42 J/g K
specificheat_copper 0.39 J/g K
specificheat_gallium 0.37 J/g K
specificheat_germanium 0.32 J/g K
specificheat_gold 0.13 J/g K
specificheat_hafnium 0.14 J/g K
specificheat_indium 0.24 J/g K
specificheat_iridium 0.13 J/g K
specificheat_iron 0.45 J/g K
specificheat_lanthanum 0.195 J/g K
specificheat_lead 0.13 J/g K
specificheat_lithium 3.57 J/g K
specificheat_lutetium 0.15 J/g K
specificheat_magnesium 1.05 J/g K
specificheat_manganese 0.48 J/g K
specificheat_mercury 0.14 J/g K
specificheat_molybdenum 0.25 J/g K
specificheat_nickel 0.44 J/g K
specificheat_osmium 0.13 J/g K
specificheat_palladium 0.24 J/g K
specificheat_platinum 0.13 J/g K
specificheat_plutonum 0.13 J/g K
specificheat_potassium 0.75 J/g K
specificheat_rhenium 0.14 J/g K
specificheat_rhodium 0.24 J/g K
specificheat_rubidium 0.36 J/g K
specificheat_ruthenium 0.24 J/g K
specificheat_scandium 0.57 J/g K
specificheat_selenium 0.32 J/g K
specificheat_silicon 0.71 J/g K
specificheat_silver 0.23 J/g K
specificheat_sodium 1.21 J/g K
specificheat_strontium 0.30 J/g K
specificheat_tantalum 0.14 J/g K
specificheat_thallium 0.13 J/g K
specificheat_thorium 0.13 J/g K
specificheat_tin 0.21 J/g K
specificheat_titanium 0.54 J/g K
specificheat_tungsten 0.13 J/g K
specificheat_uranium 0.12 J/g K
specificheat_vanadium 0.39 J/g K
specificheat_yttrium 0.30 J/g K
specificheat_zinc 0.39 J/g K
specificheat_zirconium 0.27 J/g K
specificheat_ethanol 2.3 J/g K
specificheat_ammonia 4.6 J/g K
specificheat_freon 0.91 J/g K # R-12 at 0 degrees Fahrenheit
specificheat_gasoline 2.22 J/g K
specificheat_iodine 2.15 J/g K
specificheat_oliveoil 1.97 J/g K
# en.wikipedia.org/wiki/Heat_capacity#Table_of_specific_heat_capacities
specificheat_hydrogen 14.3 J/g K
specificheat_helium 5.1932 J/g K
specificheat_argon 0.5203 J/g K
specificheat_tissue 3.5 J/g K
specificheat_diamond 0.5091 J/g K
specificheat_granite 0.79 J/g K
specificheat_graphite 0.71 J/g K
specificheat_ice 2.11 J/g K
specificheat_asphalt 0.92 J/g K
specificheat_brick 0.84 J/g K
specificheat_concrete 0.88 J/g K
specificheat_glass_silica 0.84 J/g K
specificheat_glass_flint 0.503 J/g K
specificheat_glass_pyrex 0.753 J/g K
specificheat_gypsum 1.09 J/g K
specificheat_marble 0.88 J/g K
specificheat_sand 0.835 J/g K
specificheat_soil 0.835 J/g K
specificheat_wood 1.7 J/g K
specificheat_sucrose 1.244 J/g K # www.sugartech.co.za/heatcapacity/indexphp
# Energy densities of various fuels
#
# Most of these fuels have varying compositions or qualities and hence their
# actual energy densities vary. These numbers are hence only approximate.
#
# E1. http://www.aps.org/policy/reports/popa-reports/energy/units.cfm
# E2. https://web.archive.org/web/20100825042309/http://www.ior.com.au/ecflist.html
tonoil 1e10 cal_IT # Ton oil equivalent. A conventional
# value for the energy released by
toe tonoil # burning one metric ton of oil. [18,E1]
# Note that energy per mass of petroleum
# products is fairly constant.
# Variations in volumetric energy
# density result from variations in the
# density (kg/m^3) of different fuels.
# This definition is given by the
# IEA/OECD.
toncoal 7e9 cal_IT # Energy in metric ton coal from [18].
# This is a nominal value which
# is close to the heat content
# of coal used in the 1950's
barreloil 5.8 Mbtu # Conventional value for barrel of crude
# oil [E1]. Actual range is 5.6 - 63.
naturalgas_HHV 1027 btu/ft3 # Energy content of natural gas. HHV
naturalgas_LHV 930 btu/ft3 # is for Higher Heating Value and
naturalgas naturalgas_HHV # includes energy from condensation
# combustion products. LHV is for Lower
# Heating Value and excludes these.
# American publications typically report
# HHV whereas European ones report LHV.
charcoal 30 GJ/tonne
woodenergy_dry 20 GJ/tonne # HHV, a cord weights about a tonne
woodenergy_airdry 15 GJ/tonne # 20% moisture content
coal_bituminous 27 GJ / tonne
coal_lignite 15 GJ / tonne
coal_US 22 GJ / uston # Average for US coal (short ton), 1995
ethanol_HHV 84000 btu/usgallon
ethanol_LHV 75700 btu/usgallon
diesel 130500 btu/usgallon
gasoline_LHV 115000 btu/usgallon
gasoline_HHV 125000 btu/usgallon
gasoline gasoline_HHV
heating 37.3 MJ/liter
fueloil 39.7 MJ/liter # low sulphur
propane 93.3 MJ/m^3
butane 124 MJ/m^3
# The US EPA defines a "miles per gallon equivalent" for alternative
# energy vehicles:
mpg_e miles / gallon gasoline_LHV
MPGe mpg_e
# These values give total energy from uranium fission. Actual efficiency
# of nuclear power plants is around 30%-40%. Note also that some reactors
# use enriched uranium around 3% U-235. Uranium during processing or use
# may be in a compound of uranium oxide or uranium hexafluoride, in which
# case the energy density would be lower depending on how much uranium is
# in the compound.
uranium_pure 200 MeV avogadro / (235.0439299 g/mol) # Pure U-235
uranium_natural 0.7% uranium_pure # Natural uranium: 0.7% U-235
# Celsius heat unit: energy to raise a pound of water 1 degC
celsiusheatunit cal lb degC / gram K
chu celsiusheatunit
# "Apparent" average power in an AC circuit, the product of rms voltage
# and rms current, equal to the true power in watts when voltage and
# current are in phase. In a DC circuit, always equal to the true power.
VA volt ampere
kWh kilowatt hour
# The horsepower is supposedly the power of one horse pulling. Obviously
# different people had different horses.
horsepower 550 foot pound force / sec # Invented by James Watt
mechanicalhorsepower horsepower
hp horsepower
metrichorsepower 75 kilogram force meter / sec # PS=Pferdestaerke in
electrichorsepower 746 W # Germany
boilerhorsepower 9809.50 W
waterhorsepower 746.043 W
brhorsepower horsepower # Value corrected Dec, 2019. Was 745.7 W.
donkeypower 250 W
chevalvapeur metrichorsepower
#
# Heat Transfer
#
# Thermal conductivity, K, measures the rate of heat transfer across
# a material. The heat transferred is
# Q = K dT A t / L
# where dT is the temperature difference across the material, A is the
# cross sectional area, t is the time, and L is the length (thickness).
# Thermal conductivity is a material property.
THERMAL_CONDUCTIVITY POWER / AREA (TEMPERATURE_DIFFERENCE/LENGTH)
THERMAL_RESISTIVITY 1/THERMAL_CONDUCTIVITY
# Thermal conductance is the rate at which heat flows across a given
# object, so the area and thickness have been fixed. It depends on
# the size of the object and is hence not a material property.
THERMAL_CONDUCTANCE POWER / TEMPERATURE_DIFFERENCE
THERMAL_RESISTANCE 1/THERMAL_CONDUCTANCE
# Thermal admittance is the rate of heat flow per area across an
# object whose thickness has been fixed. Its reciprocal, thermal
# insulation, is used to for measuring the heat transfer per area
# of sheets of insulation or cloth that are of specified thickness.
THERMAL_ADMITTANCE THERMAL_CONDUCTIVITY / LENGTH
THERMAL_INSULANCE THERMAL_RESISTIVITY LENGTH
THERMAL_INSULATION THERMAL_RESISTIVITY LENGTH
Rvalue degF ft^2 hr / btu
Uvalue 1/Rvalue
europeanUvalue watt / m^2 K
RSI degC m^2 / W
clo 0.155 degC m^2 / W # Supposed to be the insulance
# required to keep a resting person
# comfortable indoors. The value
# given is from NIST and the CRC,
# but [5] gives a slightly different
# value of 0.875 ft^2 degF hr / btu.
tog 0.1 degC m^2 / W # Also used for clothing.
# Thermal diffusivity measures the rate of heat transfer inside a
# material. It is the thermal conductivity divided by the volumentric
# heat capacity, and appears in the heat equation:
#
# du/dt = alpha (d^2 u / dx^2)
#
# where alpha is the thermal diffusivity. (Derivatives are partial derivatives.)
THERMAL_DIFFUSIVITY THERMAL_CONDUCTIVITY / DENSITY SPECIFIC_HEAT_CAPACITY
# Thermal Conductivity of a few materials
diamond_natural_thermal_conductivity 2200 W / m K
diamond_synthetic_thermal_conductivity 3320 W / m K # 99% pure C12
silver_thermal_conductivity 406 W / m K
aluminum_thermal_conductivity 205 W / m K
copper_thermal_conductivity 385 W / m K
gold_thermal_conductivity 314 W / m K
iron_thermal_conductivity 79.5 W / m K
stainless_304_thermal_conductivity 15.5 W / m K # average value
# Thermal diffusivity of a few materials
# https://en.wikipedia.org/wiki/Thermal_diffusivity
# Values for diamond from https://doi.org/10.1007/BF00351908
diamond_synthetic_thermal_diffusivity 1200 mm^2 / s
diamond_natural_thermal_diffusivity 780 mm^2 / s
helium_thermal_diffusivity 190 mm^2 / s # At 300 K, 1 atm
silver_thermal_diffusivity 165.63 mm^2 / s # 99.9% pure
gold_thermal_diffusivity 127 mm^2 / s
copper_thermal_diffusivity 111 mm^2 / s
aluminum_thermal_diffusivity 97 mm^2 / s
iron_thermal_diffusivity 23 mm^2 / s
air_thermal_diffusivity 19 mm^2 / s
stainless_304_thermal_diffusivity 4.2 mm^2 / s
ice_thermal_diffusivity 1.02 mm^2 / s # At 0 C
glass_thermal_diffusivity 0.34 mm^2 / s
water_thermal_diffusivity 0.143 mm^2 / s # At 25 C
nylon_thermal_diffusivity 0.09 mm^2 / s
pine_thermal_diffusivity 0.082 mm^2 / s # yellow pine
# The bel was defined by engineers of Bell Laboratories to describe the
# reduction in audio level over a length of one mile. It was originally
# called the transmission unit (TU) but was renamed around 1923 to honor
# Alexander Graham Bell. The bel proved inconveniently large so the decibel
# has become more common. The decibel is dimensionless since it reports a
# ratio, but it is used in various contexts to report a signal's power
# relative to some reference level.
bel(x) units=[1;1] range=(0,) 10^(x); log(bel) # Basic bel definition
decibel(x) units=[1;1] range=(0,) 10^(x/10); 10 log(decibel) # Basic decibel
dB() decibel # Abbreviation
dBW(x) units=[1;W] range=(0,) dB(x) W ; ~dB(dBW/W) # Reference = 1 W
dBk(x) units=[1;W] range=(0,) dB(x) kW ; ~dB(dBk/kW) # Reference = 1 kW
dBf(x) units=[1;W] range=(0,) dB(x) fW ; ~dB(dBf/fW) # Reference = 1 fW
dBm(x) units=[1;W] range=(0,) dB(x) mW ; ~dB(dBm/mW) # Reference = 1 mW
dBmW(x) units=[1;W] range=(0,) dBm(x) ; ~dBm(dBmW) # Reference = 1 mW
dBJ(x) units=[1;J] range=(0,) dB(x) J; ~dB(dBJ/J) # Energy relative
# to 1 joule. Used for power spectral
# density since W/Hz = J
# When used to measure amplitude, voltage, or current the signal is squared
# because power is proportional to the square of these measures. The root
# mean square (RMS) voltage is typically used with these units.
dB_amplitude(x) units=[1;1] dB(0.5 x) ; ~dB(dB_amplitude^2)
dBV(x) units=[1;V] range=(0,) dB(0.5 x) V;~dB(dBV^2 / V^2) # Reference = 1 V
dBmV(x) units=[1;V] range=(0,) dB(0.5 x) mV;~dB(dBmV^2/mV^2)# Reference = 1 mV
dBuV(x) units=[1;V] range=(0,) dB(0.5 x) microV ; ~dB(dBuV^2 / microV^2)
# Reference = 1 microvolt
# Here are dB measurements for current. Be aware that dbA is also
# a unit for frequency weighted sound pressure.
dBA(x) units=[1;A] range=(0,) dB(0.5 x) A;~dB(dBA^2 / A^2) # Reference = 1 A
dBmA(x) units=[1;A] range=(0,) dB(0.5 x) mA;~dB(dBmA^2/mA^2)# Reference = 1 mA
dBuA(x) units=[1;A] range=(0,) dB(0.5 x) microA ; ~dB(dBuA^2 / microA^2)
# Reference = 1 microamp
# Referenced to the voltage that causes 1 mW dissipation in a 600 ohm load.
# Originally defined as dBv but changed to prevent confusion with dBV.
# The "u" is for unloaded.
dBu(x) units=[1;V] range=(0,) dB(0.5 x) sqrt(mW 600 ohm) ; \
~dB(dBu^2 / mW 600 ohm)
dBv(x) units=[1;V] range=(0,) dBu(x) ; ~dBu(dBv) # Synonym for dBu
# Measurements for sound in air, referenced to the threshold of human hearing
# Note that sound in other media typically uses 1 micropascal as a reference
# for sound pressure. Units dBA, dBB, dBC, refer to different frequency
# weightings meant to approximate the human ear's response.
# sound pressure level
dBSPL(x) units=[1;Pa] range=(0,) dB(0.5 x) 20 microPa ; \
~dB(dBSPL^2 / (20 microPa)^2)
# sound intensity level
dBSIL(x) units=[1;W/m^2] range=(0,) dB(x) 1e-12 W/m^2; \
~dB(dBSIL / (1e-12 W/m^2))
# sound power level (The W in SWL is for the reference power, 1 W.)
dBSWL(x) units=[1;W] range=(0,) dB(x) 1e-12 W; ~dB(dBSWL/1e-12 W)
# The neper is another similar logarithmic unit. Note that the neper
# is defined based on the ratio of amplitudes rather than the power
# ratio like the decibel. This means that if the data is power, and
# you convert to nepers you should take the square root of the data
# to convert to amplitude. If you want to convert nepers to a power
# measurement you need to square the resulting output.
neper(x) units=[1;1] range=(0,) exp(x); ln(neper)
centineper(x) units=[1;1] range=(0,) exp(x/100); 100 ln(centineper)
Np() neper
cNp() centineper
Np_power(x) units=[1;1] Np(2 x) ; ~Np(Np_power)/2
# Misc other measures
ENTROPY ENERGY / TEMPERATURE
clausius 1e3 cal/K # A unit of physical entropy
langley thermcalorie/cm^2 # Used in radiation theory
poncelet 100 kg force m / s
tonrefrigeration uston 144 btu / lb day # One ton refrigeration is
# the rate of heat extraction required
# turn one ton of water to ice in
# a day. Ice is defined to have a
# latent heat of 144 btu/lb.
tonref tonrefrigeration
refrigeration tonref / ton
frigorie 1000 cal_15 # Used in refrigeration engineering.
airwatt 8.5 (ft^3/min) inH2O # Measure of vacuum power as
# pressure times air flow.
# The unit "tnt" is defined so that you can write "tons tnt". The
# question of which ton, exactly, is intended. The answer is that
# nobody knows:
#
# Quoting the footnote from page 13 of
# The Effects of Nuclear Weapons, 3rd ed.
# https://www.fourmilab.ch/etexts/www/effects/eonw_1.pdf
#
# The majority of the experimental and theoretical values of the
# explosive energy released by TNT range from 900 to 1,100 calories per
# gram. At one time, there was some uncertainty as to whether the term
# "kiloton" of TNT referred to a short kiloton (2*10^6 pounds), a metric
# kiloton (2.205*10^6 pounds), or a long kiloton (2.24*10^6 pounds). In
# order to avoid ambiguity, it was agreed that the term "kiloton" would
# refer to the release of 10^12 calories of explosive energy. This is
# equivalent to 1 short kiloton of TNT if the energy release is 1,102
# calories per gram or to 1 long kiloton if the energy is 984 calories
# per gram of TNT.
#
# It is therefore not well-defined how much energy a "gram of tnt" is,
# though this term does appear in some references.
tnt 1e9 cal_th / ton # Defined exact value
# Nuclear weapon yields
davycrocket 10 ton tnt # lightest US tactical nuclear weapon
hiroshima 15.5 kiloton tnt # Uranium-235 fission bomb
nagasaki 21 kiloton tnt # Plutonium-239 fission bomb
fatman nagasaki
littleboy hiroshima
ivyking 500 kiloton tnt # most powerful fission bomb
castlebravo 15 megaton tnt # most powerful US test
tsarbomba 50 megaton tnt # most powerful test ever: USSR,
# 30 October 1961
b53bomb 9 megaton tnt
# http://rarehistoricalphotos.com/gadget-first-atomic-bomb/
trinity 18 kiloton tnt # July 16, 1945
gadget trinity
#
# Permeability: The permeability or permeance, n, of a substance determines
# how fast vapor flows through the substance. The formula W = n A dP
# holds where W is the rate of flow (in mass/time), n is the permeability,
# A is the area of the flow path, and dP is the vapor pressure difference.
#
perm_0C grain / hr ft^2 inHg
perm_zero perm_0C
perm_0 perm_0C
perm perm_0C
perm_23C grain / hr ft^2 in Hg23C
perm_twentythree perm_23C
#
# Counting measures
#
pair 2
brace 2
nest 3 # often used for items like bowls that
# nest together
hattrick 3 # Used in sports, especially cricket and ice
# hockey to report the number of goals.
dicker 10
dozen 12
bakersdozen 13
score 20
flock 40
timer 40
shock 60
toncount 100 # Used in sports in the UK
longhundred 120 # From a germanic counting system
gross 144
greatgross 12 gross
tithe 1|10 # From Anglo-Saxon word for tenth
# Paper counting measure
shortquire 24
quire 25
shortream 480
ream 500
perfectream 516
bundle 2 reams
bale 5 bundles
#
# Paper measures
#
# USA paper sizes
lettersize 8.5 inch 11 inch
legalsize 8.5 inch 14 inch
ledgersize 11 inch 17 inch
executivesize 7.25 inch 10.5 inch
Apaper 8.5 inch 11 inch
Bpaper 11 inch 17 inch
Cpaper 17 inch 22 inch
Dpaper 22 inch 34 inch
Epaper 34 inch 44 inch
# Correspondence envelope sizes. #10 is the standard business
# envelope in the USA.
envelope6_25size 3.5 inch 6 inch
envelope6_75size 3.625 inch 6.5 inch
envelope7size 3.75 inch 6.75 inch
envelope7_75size 3.875 inch 7.5 inch
envelope8_625size 3.625 inch 8.625 inch
envelope9size 3.875 inch 8.875 inch
envelope10size 4.125 inch 9.5 inch
envelope11size 4.5 inch 10.375 inch
envelope12size 4.75 inch 11 inch
envelope14size 5 inch 11.5 inch
envelope16size 6 inch 12 inch
# Announcement envelope sizes (no relation to metric paper sizes like A4)
envelopeA1size 3.625 inch 5.125 inch # same as 4bar
envelopeA2size 4.375 inch 5.75 inch
envelopeA6size 4.75 inch 6.5 inch
envelopeA7size 5.25 inch 7.25 inch
envelopeA8size 5.5 inch 8.125 inch
envelopeA9size 5.75 inch 8.75 inch
envelopeA10size 6 inch 9.5 inch
# Baronial envelopes
envelope4bar 3.625 inch 5.125 inch # same as A1
envelope5_5bar 4.375 inch 5.75 inch
envelope6bar 4.75 inch 6.5 inch
# Coin envelopes
envelope1baby 2.25 inch 3.5 inch # same as #1 coin
envelope00coin 1.6875 inch 2.75 inch
envelope1coin 2.25 inch 3.5 inch
envelope3coin 2.5 inch 4.25 inch
envelope4coin 3 inch 4.5 inch
envelope4_5coin 3 inch 4.875 inch
envelope5coin 2.875 inch 5.25 inch
envelope5_5coin 3.125 inch 5.5 inch
envelope6coin 3.375 inch 6 inch
envelope7coin 3.5 inch 6.5 inch
# The metric paper sizes are defined so that if a sheet is cut in half
# along the short direction, the result is two sheets which are
# similar to the original sheet. This means that for any metric size,
# the long side is close to sqrt(2) times the length of the short
# side. Each series of sizes is generated by repeated cuts in half,
# with the values rounded down to the nearest millimeter.
A0paper 841 mm 1189 mm # The basic size in the A series
A1paper 594 mm 841 mm # is defined to have an area of
A2paper 420 mm 594 mm # one square meter.
A3paper 297 mm 420 mm
A4paper 210 mm 297 mm
A5paper 148 mm 210 mm
A6paper 105 mm 148 mm
A7paper 74 mm 105 mm
A8paper 52 mm 74 mm
A9paper 37 mm 52 mm
A10paper 26 mm 37 mm
B0paper 1000 mm 1414 mm # The basic B size has an area
B1paper 707 mm 1000 mm # of sqrt(2) square meters.
B2paper 500 mm 707 mm
B3paper 353 mm 500 mm
B4paper 250 mm 353 mm
B5paper 176 mm 250 mm
B6paper 125 mm 176 mm
B7paper 88 mm 125 mm
B8paper 62 mm 88 mm
B9paper 44 mm 62 mm
B10paper 31 mm 44 mm
C0paper 917 mm 1297 mm # The basic C size has an area
C1paper 648 mm 917 mm # of sqrt(sqrt(2)) square meters.
C2paper 458 mm 648 mm
C3paper 324 mm 458 mm # Intended for envelope sizes
C4paper 229 mm 324 mm
C5paper 162 mm 229 mm
C6paper 114 mm 162 mm
C7paper 81 mm 114 mm
C8paper 57 mm 81 mm
C9paper 40 mm 57 mm
C10paper 28 mm 40 mm
# gsm (Grams per Square Meter), a sane, metric paper weight measure
gsm grams / meter^2
# In the USA, a collection of crazy historical paper measures are used. Paper
# is measured as a weight of a ream of that particular type of paper. This is
# sometimes called the "substance" or "basis" (as in "substance 20" paper).
# The standard sheet size or "basis size" varies depending on the type of
# paper. As a result, 20 pound bond paper and 50 pound text paper are actually
# about the same weight. The different sheet sizes were historically the most
# convenient for printing or folding in the different applications. These
# different basis weights are standards maintained by American Society for
# Testing Materials (ASTM) and the American Forest and Paper Association
# (AF&PA).
poundbookpaper lb / 25 inch 38 inch ream
lbbook poundbookpaper
poundtextpaper poundbookpaper
lbtext poundtextpaper
poundoffsetpaper poundbookpaper # For offset printing
lboffset poundoffsetpaper
poundbiblepaper poundbookpaper # Designed to be lightweight, thin,
lbbible poundbiblepaper # strong and opaque.
poundtagpaper lb / 24 inch 36 inch ream
lbtag poundtagpaper
poundbagpaper poundtagpaper
lbbag poundbagpaper
poundnewsprintpaper poundtagpaper
lbnewsprint poundnewsprintpaper
poundposterpaper poundtagpaper
lbposter poundposterpaper
poundtissuepaper poundtagpaper
lbtissue poundtissuepaper
poundwrappingpaper poundtagpaper
lbwrapping poundwrappingpaper
poundwaxingpaper poundtagpaper
lbwaxing poundwaxingpaper
poundglassinepaper poundtagpaper
lbglassine poundglassinepaper
poundcoverpaper lb / 20 inch 26 inch ream
lbcover poundcoverpaper
poundindexpaper lb / 25.5 inch 30.5 inch ream
lbindex poundindexpaper
poundindexbristolpaper poundindexpaper
lbindexbristol poundindexpaper
poundbondpaper lb / 17 inch 22 inch ream # Bond paper is stiff and
lbbond poundbondpaper # durable for repeated
poundwritingpaper poundbondpaper # filing, and it resists
lbwriting poundwritingpaper # ink penetration.
poundledgerpaper poundbondpaper
lbledger poundledgerpaper
poundcopypaper poundbondpaper
lbcopy poundcopypaper
poundblottingpaper lb / 19 inch 24 inch ream
lbblotting poundblottingpaper
poundblankspaper lb / 22 inch 28 inch ream
lbblanks poundblankspaper
poundpostcardpaper lb / 22.5 inch 28.5 inch ream
lbpostcard poundpostcardpaper
poundweddingbristol poundpostcardpaper
lbweddingbristol poundweddingbristol
poundbristolpaper poundweddingbristol
lbbristol poundbristolpaper
poundboxboard lb / 1000 ft^2
lbboxboard poundboxboard
poundpaperboard poundboxboard
lbpaperboard poundpaperboard
# When paper is marked in units of M, it means the weight of 1000 sheets of the
# given size of paper. To convert this to paper weight, divide by the size of
# the paper in question.
paperM lb / 1000
# In addition paper weight is reported in "caliper" which is simply the
# thickness of one sheet, typically in inches. Thickness is also reported in
# "points" where a point is 1|1000 inch. These conversions are supplied to
# convert these units roughly (using an approximate density) into the standard
# paper weight values.
pointthickness 0.001 in
paperdensity 0.8 g/cm^3 # approximate--paper densities vary!
papercaliper in paperdensity
paperpoint pointthickness paperdensity
#
# Printing
#
fournierpoint 0.1648 inch / 12 # First definition of the printers
# point made by Pierre Fournier who
# defined it in 1737 as 1|12 of a
# cicero which was 0.1648 inches.
olddidotpoint 1|72 frenchinch # Francois Ambroise Didot, one of
# a family of printers, changed
# Fournier's definition around 1770
# to fit to the French units then in
# use.
bertholdpoint 1|2660 m # H. Berthold tried to create a
# metric version of the didot point
# in 1878.
INpoint 0.4 mm # This point was created by a
# group directed by Fermin Didot in
# 1881 and is associated with the
# imprimerie nationale. It doesn't
# seem to have been used much.
germandidotpoint 0.376065 mm # Exact definition appears in DIN
# 16507, a German standards document
# of 1954. Adopted more broadly in
# 1966 by ???
metricpoint 3|8 mm # Proposed in 1977 by Eurograf
oldpoint 1|72.27 inch # The American point was invented
printerspoint oldpoint # by Nelson Hawks in 1879 and
texpoint oldpoint # dominates USA publishing.
# It was standardized by the American
# Typefounders Association at the
# value of 0.013837 inches exactly.
# Knuth uses the approximation given
# here (which is very close). The
# comp.fonts FAQ claims that this
# value is supposed to be 1|12 of a
# pica where 83 picas is equal to 35
# cm. But this value differs from
# the standard.
texscaledpoint 1|65536 texpoint # The TeX typesetting system uses
texsp texscaledpoint # this for all computations.
computerpoint 1|72 inch # The American point was rounded
point computerpoint
computerpica 12 computerpoint # to an even 1|72 inch by computer
postscriptpoint computerpoint # people at some point.
pspoint postscriptpoint
twip 1|20 point # TWentieth of an Imperial Point
Q 1|4 mm # Used in Japanese phototypesetting
# Q is for quarter
frenchprinterspoint olddidotpoint
didotpoint germandidotpoint # This seems to be the dominant value
europeanpoint didotpoint # for the point used in Europe
cicero 12 didotpoint
stick 2 inches
# Type sizes
excelsior 3 oldpoint
brilliant 3.5 oldpoint
diamondtype 4 oldpoint
pearl 5 oldpoint
agate 5.5 oldpoint # Originally agate type was 14 lines per
# inch, giving a value of 1|14 in.
ruby agate # British
nonpareil 6 oldpoint
mignonette 6.5 oldpoint
emerald mignonette # British
minion 7 oldpoint
brevier 8 oldpoint
bourgeois 9 oldpoint
longprimer 10 oldpoint
smallpica 11 oldpoint
pica 12 oldpoint
english 14 oldpoint
columbian 16 oldpoint
greatprimer 18 oldpoint
paragon 20 oldpoint
meridian 44 oldpoint
canon 48 oldpoint
# German type sizes
nonplusultra 2 didotpoint
brillant 3 didotpoint
diamant 4 didotpoint
perl 5 didotpoint
nonpareille 6 didotpoint
kolonel 7 didotpoint
petit 8 didotpoint
borgis 9 didotpoint
korpus 10 didotpoint
corpus korpus
garamond korpus
mittel 14 didotpoint
tertia 16 didotpoint
text 18 didotpoint
kleine_kanon 32 didotpoint
kanon 36 didotpoint
grobe_kanon 42 didotpoint
missal 48 didotpoint
kleine_sabon 72 didotpoint
grobe_sabon 84 didotpoint
#
# Information theory units. Note that the name "entropy" is used both
# to measure information and as a physical quantity.
#
INFORMATION bit
nat (1/ln(2)) bits # Entropy measured base e
hartley log2(10) bits # Entropy of a uniformly
ban hartley # distributed random variable
# over 10 symbols.
dit hartley # from Decimal digIT
#
# Computer
#
bps bit/sec # Sometimes the term "baud" is
# incorrectly used to refer to
# bits per second. Baud refers
# to symbols per second. Modern
# modems transmit several bits
# per symbol.
byte 8 bit # Not all machines had 8 bit
B byte # bytes, but these days most of
# them do. But beware: for
# transmission over modems, a
# few extra bits are used so
# there are actually 10 bits per
# byte.
octet 8 bits # The octet is always 8 bits
nybble 4 bits # Half of a byte. Sometimes
# equal to different lengths
# such as 3 bits.
nibble nybble
nyp 2 bits # Donald Knuth asks in an exercise
# for a name for a 2 bit
# quantity and gives the "nyp"
# as a solution due to Gregor
# Purdy. Not in common use.
meg megabyte # Some people consider these
# units along with the kilobyte
gig gigabyte # to be defined according to
# powers of 2 with the kilobyte
# equal to 2^10 bytes, the
# megabyte equal to 2^20 bytes and
# the gigabyte equal to 2^30 bytes
# but these usages are forbidden
# by SI. Binary prefixes have
# been defined by IEC to replace
# the SI prefixes. Use them to
# get the binary units KiB, MiB,
# GiB, etc.
jiffy 0.01 sec # This is defined in the Jargon File
jiffies jiffy # (http://www.jargon.org) as being the
# duration of a clock tick for measuring
# wall-clock time. Supposedly the value
# used to be 1|60 sec or 1|50 sec
# depending on the frequency of AC power,
# but then 1|100 sec became more common.
# On linux systems, this term is used and
# for the Intel based chips, it does have
# the value of .01 sec. The Jargon File
# also lists two other definitions:
# millisecond, and the time taken for
# light to travel one foot.
cdaudiospeed 44.1 kHz 2*16 bits # CD audio data rate at 44.1 kHz with 2
# samples of sixteen bits each.
cdromspeed 75 2048 bytes / sec # For data CDs (mode1) 75 sectors are read
# each second with 2048 bytes per sector.
# Audio CDs do not have sectors, but
# people sometimes divide the bit rate by
# 75 and claim a sector length of 2352.
# Data CDs have a lower rate due to
# increased error correction overhead.
# There is a rarely used mode (mode2) with
# 2336 bytes per sector that has fewer
# error correction bits than mode1.
dvdspeed 1385 kB/s # This is the "1x" speed of a DVD using
# constant linear velocity (CLV) mode.
# Modern DVDs may vary the linear velocity
# as they go from the inside to the
# outside of the disc.
# See http://www.osta.org/technology/dvdqa/dvdqa4.htm
FIT / 1e9 hour # Failures In Time, number of failures per billion hours
#
# The IP address space is divided into subnets. The number of hosts
# in a subnet depends on the length of the subnet prefix. This is
# often written as /N where N is the number of bits in the prefix.
#
# https://en.wikipedia.org/wiki/Subnetwork
#
# These definitions gives the number of hosts for a subnet whose
# prefix has the specified length in bits.
#
ipv4subnetsize(prefix_len) units=[1;1] domain=[0,32] range=[1,4294967296] \
2^(32-prefix_len) ; 32-log2(ipv4subnetsize)
ipv4classA ipv4subnetsize(8)
ipv4classB ipv4subnetsize(16)
ipv4classC ipv4subnetsize(24)
ipv6subnetsize(prefix_len) units=[1;1] domain=[0,128] \
range=[1,340282366920938463463374607431768211456] \
2^(128-prefix_len) ; 128-log2(ipv6subnetsize)
#
# Musical measures. Musical intervals expressed as ratios. Multiply
# two intervals together to get the sum of the interval. The function
# musicalcent can be used to convert ratios to cents.
#
# Perfect intervals
octave 2
majorsecond musicalfifth^2 / octave
majorthird 5|4
minorthird 6|5
musicalfourth 4|3
musicalfifth 3|2
majorsixth musicalfourth majorthird
minorsixth musicalfourth minorthird
majorseventh musicalfifth majorthird
minorseventh musicalfifth minorthird
pythagoreanthird majorsecond musicalfifth^2 / octave
syntoniccomma pythagoreanthird / majorthird
pythagoreancomma musicalfifth^12 / octave^7
# Equal tempered definitions
semitone octave^(1|12)
musicalcent(x) units=[1;1] range=(0,) semitone^(x/100) ; \
100 log(musicalcent)/log(semitone)
#
# Musical note lengths.
#
wholenote !
MUSICAL_NOTE_LENGTH wholenote
halfnote 1|2 wholenote
quarternote 1|4 wholenote
eighthnote 1|8 wholenote
sixteenthnote 1|16 wholenote
thirtysecondnote 1|32 wholenote
sixtyfourthnote 1|64 wholenote
dotted 3|2
doubledotted 7|4
breve doublewholenote
semibreve wholenote
minimnote halfnote
crotchet quarternote
quaver eighthnote
semiquaver sixteenthnote
demisemiquaver thirtysecondnote
hemidemisemiquaver sixtyfourthnote
semidemisemiquaver hemidemisemiquaver
#
# yarn and cloth measures
#
# yarn linear density
woolyarnrun 1600 yard/pound # 1600 yds of "number 1 yarn" weighs
# a pound.
yarncut 300 yard/pound # Less common system used in
# Pennsylvania for wool yarn
cottonyarncount 840 yard/pound
linenyarncount 300 yard/pound # Also used for hemp and ramie
worstedyarncount 1680 ft/pound
metricyarncount meter/gram
denier 1|9 tex # used for silk and rayon
manchesteryarnnumber drams/1000 yards # old system used for silk
pli lb/in
typp 1000 yd/lb # abbreviation for Thousand Yard Per Pound
asbestoscut 100 yd/lb # used for glass and asbestos yarn
tex gram / km # rational metric yarn measure, meant
drex 0.1 tex # to be used for any kind of yarn
poumar lb / 1e6 yard
# yarn and cloth length
skeincotton 80*54 inch # 80 turns of thread on a reel with a
# 54 in circumference (varies for other
# kinds of thread)
cottonbolt 120 ft # cloth measurement
woolbolt 210 ft
bolt cottonbolt
heer 600 yards
cut 300 yards # used for wet-spun linen yarn
lea 300 yards
sailmakersyard 28.5 in
sailmakersounce oz / sailmakersyard 36 inch
silkmomme momme / 25 yards 1.49 inch # Traditional silk weight
silkmm silkmomme # But it is also defined as
# lb/100 yd 45 inch. The two
# definitions are slightly different
# and neither one seems likely to be
# the true source definition.
#
# drug dosage
#
mcg microgram # Frequently used for vitamins
iudiptheria 62.8 microgram # IU is for international unit
iupenicillin 0.6 microgram
iuinsulin 41.67 microgram
drop 1|20 ml # The drop was an old "unit" that was
# replaced by the minim. But I was
# told by a pharmacist that in his
# profession, the conversion of 20
# drops per ml is actually used.
bloodunit 450 ml # For whole blood. For blood
# components, a blood unit is the
# quantity of the component found in a
# blood unit of whole blood. The
# human body contains about 12 blood
# units of whole blood.
#
# misc medical measure
#
frenchcathetersize 1|3 mm # measure used for the outer diameter
# of a catheter
charriere frenchcathetersize
#
# fixup units for times when prefix handling doesn't do the job
#
hectare hectoare
hektare hectoare
decare dekaare
dekare dekaare
megohm megaohm
kilohm kiloohm
microhm microohm
megalerg megaerg # 'L' added to make it pronounceable [18].
#
# Money
#
# Note that US$ is the primitive unit so other currencies are
# generally given in US$.
#
unitedstatesdollar US$
usdollar US$
$ dollar
mark germanymark
#bolivar venezuelabolivar # Not all databases are
#venezuelabolivarfuerte 1e-5 bolivar # supplying these
#bolivarfuerte 1e-5 bolivar # The currency was revalued
#oldbolivar 1|1000 bolivarfuerte # twice
peseta spainpeseta
rand southafricarand
escudo portugalescudo
guilder netherlandsguilder
hollandguilder netherlandsguilder
peso mexicopeso
yen japanyen
lira turkeylira
rupee indiarupee
drachma greecedrachma
franc francefranc
markka finlandmarkka
britainpound unitedkingdompound
greatbritainpound unitedkingdompound
unitedkingdompound ukpound
poundsterling britainpound
yuan chinayuan
# Unicode Currency Names
!utf8
icelandkróna icelandkrona
polandzłoty polandzloty
tongapa’anga tongapa'anga
#venezuelabolívar venezuelabolivar
vietnamđồng vietnamdong
mongoliatögrög mongoliatugrik
sãotomé&príncipedobra saotome&principedobra
!endutf8
UKP GBP # Not an ISO code, but looks like one, and
# sometimes used on usenet.
!include currency.units
# Money on the gold standard, used in the late 19th century and early
# 20th century.
olddollargold 23.22 grains goldprice # Used until 1934
newdollargold 96|7 grains goldprice # After Jan 31, 1934
dollargold newdollargold
poundgold 113 grains goldprice # British pound
# Precious metals
goldounce goldprice troyounce
silverounce silverprice troyounce
platinumounce platinumprice troyounce
XAU goldounce
XPT platinumounce
XAG silverounce
# Nominal masses of US coins. Note that dimes, quarters and half dollars
# have weight proportional to value. Before 1965 it was $40 / kg.
USpennyweight 2.5 grams # Since 1982, 48 grains before
USnickelweight 5 grams
USdimeweight US$ 0.10 / (20 US$ / lb) # Since 1965
USquarterweight US$ 0.25 / (20 US$ / lb) # Since 1965
UShalfdollarweight US$ 0.50 / (20 US$ / lb) # Since 1971
USdollarweight 8.1 grams # Weight of Susan B. Anthony and
# Sacagawea dollar coins
# British currency
quid britainpound # Slang names
fiver 5 quid
tenner 10 quid
monkey 500 quid
brgrand 1000 quid
bob shilling
shilling 1|20 britainpound # Before decimalisation, there
oldpence 1|12 shilling # were 20 shillings to a pound,
farthing 1|4 oldpence # each of twelve old pence
guinea 21 shilling # Still used in horse racing
crown 5 shilling
florin 2 shilling
groat 4 oldpence
tanner 6 oldpence
brpenny 0.01 britainpound
pence brpenny
tuppence 2 pence
tuppenny tuppence
ha'penny halfbrpenny
hapenny ha'penny
oldpenny oldpence
oldtuppence 2 oldpence
oldtuppenny oldtuppence
threepence 3 oldpence # threepence never refers to new money
threepenny threepence
oldthreepence threepence
oldthreepenny threepence
oldhalfpenny halfoldpenny
oldha'penny oldhalfpenny
oldhapenny oldha'penny
brpony 25 britainpound
# Canadian currency
loony 1 canadadollar # This coin depicts a loon
toony 2 canadadollar
# Cryptocurrency
satoshi 1e-8 bitcoin
XBT bitcoin # nonstandard code
# Inflation.
#
# Currently US inflation as reported by the BLS CPI index is available.
# The UScpi() table reports the USA consumer price index. Note that
# if you specify a year like 2015, that refers to the CPI reported
# for December of 2014 (which is released in mid January 2015),
# so it refers to the point right at the start of the given year.
# Months are increments of 1|12 on the year, so the January 2015
# release will be 2015+1|12 = 2015.08333.
!include cpi.units
USCPI() UScpi
USCPI_now UScpi_now
USCPI_lastdate UScpi_lastdate
cpi() UScpi
CPI() UScpi
cpi_now UScpi_now
CPI_now UScpi_now
cpi_lastdate UScpi_lastdate
CPI_lastdate UScpi_lastdate
# These definitions hide the CPI index and directly convert US dollars
# from a specified date to current dollars. You can use this to convert
# historical dollars to present value or to convert money in the past
# between two dates.
dollars_in() USdollars_in
US$in() USdollars_in
$in() USdollars_in
# This definition gives the dimensionless US inflation factor since the
# specified date.
inflation_since() USinflation_since
#
# Units used for measuring volume of wood
#
cord 4*4*8 ft^3 # 4 ft by 4 ft by 8 ft bundle of wood
facecord 1|2 cord
cordfoot 1|8 cord # One foot long section of a cord
cordfeet cordfoot
housecord 1|3 cord # Used to sell firewood for residences,
# often confusingly called a "cord"
boardfoot ft^2 inch # Usually 1 inch thick wood
boardfeet boardfoot
fbm boardfoot # feet board measure
stack 4 yard^3 # British, used for firewood and coal [18]
rick 4 ft 8 ft 16 inches # Stack of firewood, supposedly
# sometimes called a face cord, but this
# value is equal to 1|3 cord. Name
# comes from an old Norse word for a
# stack of wood.
stere m^3
timberfoot ft^3 # Used for measuring solid blocks of wood
standard 120 12 ft 11 in 1.5 in # This is the St Petersburg or
# Pittsburg standard. Apparently the
# term is short for "standard hundred"
# which was meant to refer to 100 pieces
# of wood (deals). However, this
# particular standard is equal to 120
# deals which are 12 ft by 11 in by 1.5
# inches (not the standard deal).
hoppusfoot (4/pi) ft^3 # Volume calculation suggested in 1736
hoppusboardfoot 1|12 hoppusfoot # forestry manual by Edward Hoppus, for
hoppuston 50 hoppusfoot # estimating the usable volume of a log.
# It results from computing the volume
# of a cylindrical log of length, L, and
# girth (circumference), G, by V=L(G/4)^2.
# The hoppus ton is apparently still in
# use for shipments from Southeast Asia.
# In Britain, the deal is apparently any piece of wood over 6 feet long, over
# 7 wide and 2.5 inches thick. The OED doesn't give a standard size. A piece
# of wood less than 7 inches wide is called a "batten". This unit is now used
# exclusively for fir and pine.
deal 12 ft 11 in 2.5 in # The standard North American deal [OED]
wholedeal 12 ft 11 in 1.25 in # If it's half as thick as the standard
# deal it's called a "whole deal"!
splitdeal 12 ft 11 in 5|8 in # And half again as thick is a split deal.
# Used for shellac mixing rate
poundcut pound / gallon
lbcut poundcut
#
# Gas and Liquid flow units
#
FLUID_FLOW VOLUME / TIME
# Some obvious volumetric gas flow units (cu is short for cubic)
cumec m^3/s
cusec ft^3/s
# Conventional abbreviations for fluid flow units
gph gal/hr
gpm gal/min
mgd megagal/day
brgph brgallon/hr
brgpm brgallon/min
brmgd mega brgallon/day
usgph usgallon/hr
usgpm usgallon/min
usmgd mega usgallon/day
cfs ft^3/s
cfh ft^3/hour
cfm ft^3/min
lpm liter/min
lfm ft/min # Used to report air flow produced by fans.
# Multiply by cross sectional area to get a
# flow in cfm.
pru mmHg / (ml/min) # peripheral resistance unit, used in
# medicine to assess blood flow in
# the capillaries.
# Miner's inch: This is an old historic unit used in the Western United
# States. It is generally defined as the rate of flow through a one square
# inch hole at a specified depth such as 4 inches. In the late 19th century,
# volume of water was sometimes measured in the "24 hour inch". Values for the
# miner's inch were fixed by state statues. (This information is from a web
# site operated by the Nevada Division of Water Planning: The Water Words
# Dictionary at http://water.nv.gov/WaterPlanDictionary.aspx, specifically
# http://water.nv.gov/programs/planning/dictionary/wwords-M.pdf. All
# but minersinchNV are s.v. Miner's Inch [Western United States])
minersinchAZ 1.5 ft^3/min
minersinchCA 1.5 ft^3/min
minersinchMT 1.5 ft^3/min
minersinchNV 1.5 ft^3/min
minersinchOR 1.5 ft^3/min
minersinchID 1.2 ft^3/min
minersinchKS 1.2 ft^3/min
minersinchNE 1.2 ft^3/min
minersinchNM 1.2 ft^3/min
minersinchND 1.2 ft^3/min
minersinchSD 1.2 ft^3/min
minersinchUT 1.2 ft^3/min
minersinchCO 1 ft^3/sec / 38.4 # 38.4 miner's inches = 1 ft^3/sec
minersinchBC 1.68 ft^3/min # British Columbia
# Oceanographic flow
sverdrup 1e6 m^3 / sec # Used to express flow of ocean
# currents. Named after Norwegian
# oceanographer H. Sverdrup.
# In vacuum science and some other applications, gas flow is measured
# as the product of volumetric flow and pressure. This is useful
# because it makes it easy to compare with the flow at standard
# pressure (one atmosphere). It also directly relates to the number
# of gas molecules per unit time, and hence to the mass flow if the
# molecular mass is known.
GAS_FLOW PRESSURE FLUID_FLOW
sccm atm cc/min # 's' is for "standard" to indicate
sccs atm cc/sec # flow at standard pressure
scfh atm ft^3/hour #
scfm atm ft^3/min
slpm atm liter/min
slph atm liter/hour
lusec liter micron Hg / s # Used in vacuum science
# US Standard Atmosphere (1976)
# Atmospheric temperature and pressure vs. geometric height above sea level
# This definition covers only the troposphere (the lowest atmospheric
# layer, up to 11 km), and assumes the layer is polytropic.
# A polytropic process is one for which PV^k = const, where P is the
# pressure, V is the volume, and k is the polytropic exponent. The
# polytropic index is n = 1 / (k - 1). As noted in the Wikipedia article
# https://en.wikipedia.org/wiki/Polytropic_process, some authors reverse
# the definitions of "exponent" and "index." The functions below assume
# the following parameters:
# temperature lapse rate, -dT/dz, in troposphere
lapserate 6.5 K/km # US Std Atm (1976)
# air molecular weight, including constituent mol wt, given
# in Table 3, p. 3; CH4 (16.04303) and N2O (44.0128) from
# Table 15, p. 33. Values for molecular weights are slightly
# different from current values, so the original numerical
# values are retained.
air_1976 78.084 % 28.0134 \
+ 20.9476 % 31.9988 \
+ 9340 ppm 39.948 \
+ 314 ppm 44.00995 \
+ 18.18 ppm 20.183 \
+ 5.24 ppm 4.0026 \
+ 1.5 ppm 16.04303 \
+ 1.14 ppm 83.80 \
+ 0.5 ppm 2.01594 \
+ 0.27 ppm 44.0128 \
+ 0.087 ppm 131.30
# from US Standard Atmosphere, 1962, Table I.2.7, p. 9
air_1962 78.084 % 28.0134 \
+ 20.9476 % 31.9988 \
+ 9340 ppm 39.948 \
+ 314 ppm 44.00995 \
+ 18.18 ppm 20.183 \
+ 5.24 ppm 4.0026 \
+ 2 ppm 16.04303 \
+ 1.14 ppm 83.80 \
+ 0.5 ppm 2.01594 \
+ 0.5 ppm 44.0128 \
+ 0.087 ppm 131.30
# Average molecular weight of air
#
# Concentration of greenhouse gases CO2, CH4, and N20 are from
# https://gml.noaa.gov/ccgg/trends/global.html (accessed 2023-04-10);
# others are from NASA Earth Fact Sheet
# https://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html (accessed 2023-04-10)
# Numbers do not add up to exactly 100% due to roundoff and uncertainty. Water
# is highly variable, typically makes up about 1%
air_2023 78.08% nitrogen 2 \
+ 20.95% oxygen 2 \
+ 9340 ppm argon \
+ 419 ppm (carbon + oxygen 2) \
+ 18.18 ppm neon \
+ 5.24 ppm helium \
+ 1.92 ppm (carbon + 4 hydrogen) \
+ 1.14 ppm krypton \
+ 0.55 ppm hydrogen 2 \
+ 0.34 ppm (nitrogen 2 + oxygen)
# from NASA Earth Fact Sheet (accessed 28 August 2015)
# http://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html
air_2015 78.08% nitrogen 2 \
+ 20.95% oxygen 2 \
+ 9340 ppm argon \
+ 400 ppm (carbon + oxygen 2) \
+ 18.18 ppm neon \
+ 5.24 ppm helium \
+ 1.7 ppm (carbon + 4 hydrogen) \
+ 1.14 ppm krypton \
+ 0.55 ppm hydrogen 2
air air_2023
# universal gas constant
R_1976 8.31432e3 N m/(kmol K)
# polytropic index n
polyndx_1976 air_1976 (kg/kmol) gravity/(R_1976 lapserate) - 1
# If desired, redefine using current values for air mol wt and R
polyndx polyndx_1976
# polyndx air (kg/kmol) gravity/(R lapserate) - 1
# for comparison with various references
polyexpnt (polyndx + 1) / polyndx
# The model assumes the following reference values:
# sea-level temperature and pressure
stdatmT0 288.15 K
stdatmP0 atm
# "effective radius" for relation of geometric to geopotential height,
# at a latitude at which g = 9.80665 m/s (approximately 45.543 deg); no
# relation to actual radius
earthradUSAtm 6356766 m
# Temperature vs. geopotential height h
# Assumes 15 degC at sea level
# Based on approx 45 deg latitude
# Lower limits of domain and upper limits of range are those of the
# tables in US Standard Atmosphere (NASA 1976)
stdatmTH(h) units=[m;K] domain=[-5000,11e3] range=[217,321] \
stdatmT0+(-lapserate h) ; (stdatmT0+(-stdatmTH))/lapserate
# Temperature vs. geometric height z; based on approx 45 deg latitude
stdatmT(z) units=[m;K] domain=[-5000,11e3] range=[217,321] \
stdatmTH(geop_ht(z)) ; ~geop_ht(~stdatmTH(stdatmT))
# Pressure vs. geopotential height h
# Assumes 15 degC and 101325 Pa at sea level
# Based on approx 45 deg latitude
# Lower limits of domain and upper limits of range are those of the
# tables in US Standard Atmosphere (NASA 1976)
stdatmPH(h) units=[m;Pa] domain=[-5000,11e3] range=[22877,177764] \
atm (1 - (lapserate/stdatmT0) h)^(polyndx + 1) ; \
(stdatmT0/lapserate) (1+(-(stdatmPH/stdatmP0)^(1/(polyndx + 1))))
# Pressure vs. geometric height z; based on approx 45 deg latitude
stdatmP(z) units=[m;Pa] domain=[-5000,11e3] range=[22877,177764] \
stdatmPH(geop_ht(z)); ~geop_ht(~stdatmPH(stdatmP))
# Geopotential height from geometric height
# Based on approx 45 deg latitude
# Lower limits of domain and range are somewhat arbitrary; they
# correspond to the limits in the US Std Atm tables
geop_ht(z) units=[m;m] domain=[-5000,) range=[-5004,) \
(earthradUSAtm z) / (earthradUSAtm + z) ; \
(earthradUSAtm geop_ht) / (earthradUSAtm + (-geop_ht))
# The standard value for the sea-level acceleration due to gravity is
# 9.80665 m/s^2, but the actual value varies with latitude (Harrison 1949)
# R_eff = 2 g_phi / denom
# g_phi = 978.0356e-2 (1+0.0052885 sin(lat)^2+(-0.0000059) sin(2 lat)^2)
# or
# g_phi = 980.6160e-2 (1+(-0.0026373) cos(2 lat)+0.0000059 cos(2 lat)^2)
# denom = 3.085462e-6+2.27e-9 cos(2 lat)+(-2e-12) cos(4 lat) (minutes?)
# There is no inverse function; the standard value applies at a latitude
# of about 45.543 deg
g_phi(lat) units=[deg;m/s2] domain=[0,90] noerror \
980.6160e-2 (1+(-0.0026373) cos(2 lat)+0.0000059 cos(2 lat)^2) m/s2
# effective Earth radius for relation of geometric height to
# geopotential height, as function of latitude (Harrison 1949)
earthradius_eff(lat) units=[deg;m] domain=[0,90] noerror \
m 2 9.780356 (1+0.0052885 sin(lat)^2+(-0.0000059) sin(2 lat)^2) / \
(3.085462e-6 + 2.27e-9 cos(2 lat) + (-2e-12) cos(4 lat))
# References
# Harrison, L.P. 1949. Relation Between Geopotential and Geometric
# Height. In Smithsonian Meteorological Tables. List, Robert J., ed.
# 6th ed., 4th reprint, 1968. Washington, DC: Smithsonian Institution.
# NASA. US National Aeronautics and Space Administration. 1976.
# US Standard Atmosphere 1976. Washington, DC: US Government Printing Office.
# Gauge pressure functions
#
# Gauge pressure is measured relative to atmospheric pressure. In the English
# system, where pressure is often given in pounds per square inch, gauge
# pressure is often indicated by 'psig' to distinguish it from absolute
# pressure, often indicated by 'psia'. At the standard atmospheric pressure
# of 14.696 psia, a gauge pressure of 0 psig is an absolute pressure of 14.696
# psia; an automobile tire inflated to 31 psig has an absolute pressure of
# 45.696 psia.
#
# With gaugepressure(), the units must be specified (e.g., gaugepressure(1.5
# bar)); with psig(), the units are taken as psi, so the example above of tire
# pressure could be given as psig(31).
#
# If the normal elevation is significantly different from sea level, change
# Patm appropriately, and adjust the lower domain limit on the gaugepressure
# definition.
Patm atm
gaugepressure(x) units=[Pa;Pa] domain=[-101325,) range=[0,) \
x + Patm ; gaugepressure+(-Patm)
psig(x) units=[1;Pa] domain=[-14.6959487755135,) range=[0,) \
gaugepressure(x psi) ; ~gaugepressure(psig) / psi
# Pressure for underwater diving
seawater 0.1 bar / meter
msw meter seawater
fsw foot seawater
#
# Wire Gauge
#
# This area is a nightmare with huge charts of wire gauge diameters
# that usually have no clear origin. There are at least 5 competing wire gauge
# systems to add to the confusion. The use of wire gauge is related to the
# manufacturing method: a metal rod is heated and drawn through a hole. The
# size change can't be too big. To get smaller wires, the process is repeated
# with a series of smaller holes. Generally larger gauges mean smaller wires.
# The gauges often have values such as "00" and "000" which are larger sizes
# than simply "0" gauge. In the tables that appear below, these gauges must be
# specified as negative numbers (e.g. "00" is -1, "000" is -2, etc).
# Alternatively, you can use the following units:
#
g0 (0) # 1/0
g00 (-1) # 2/0
g000 (-2) # 3/0
g0000 (-3) # 4/0
g00000 (-4) # 5/0
g000000 (-5) # 6/0
g0000000 (-6) # 7/0
# or
g1_0 (-1) # 1/0
g2_0 (-1) # 2/0
g3_0 (-2) # 3/0
g4_0 (-3) # 4/0
g5_0 (-4) # 5/0
g6_0 (-5) # 6/0
g7_0 (-6) # 7/0
# American Wire Gauge (AWG), formerly known as Brown & Sharpe Gauge, appears to
# be the most important gauge. ASTM B 258 specifies that this gauge is based
# on geometric interpolation between gauge 0000, which is 0.46 inches exactly,
# and gauge 36 which is 0.005 inches exactly. Therefore, the diameter in
# inches of a wire is given by the formula 1|200 92^((36-g)/39). Note that
# 92^(1/39) is close to 2^(1/6), so diameter is approximately halved for every
# 6 gauges. For the repeated zero values, e.g., "000", use negative numbers
# (or the gxx... units) in the formula, as described above. In North America,
# sizes larger than 0000 ("4/0") are usually given in terms of circular mils,
# beginning with 250 kcmil.
#
# ASTM B 258 also specifies rounding rules which seem to be ignored by makers
# of tables. Gauges up to 44 are to be specified with up to 4 significant
# figures, but no closer than 0.0001 inch. Gauges from 44 to 56 are to be
# rounded to the nearest 0.00001 inch.
#
# In addition to being used to measure wire thickness, this gauge is used to
# measure the thickness of sheets of aluminum, copper, and most metals other
# than steel, iron and zinc.
# This converts AWG to a lineal dimension (diameter, in the case of wire).
wiregauge(g) units=[1;m] range=(0,) \
1|200 92^((36+(-g))/39) in; 36+(-39)ln(200 wiregauge/in)/ln(92)
wirega() wiregauge
awg() wiregauge
# In North America, sizes larger than 0000 AWG are usually given in area in
# kcmil (formerly, MCM). Outside North America, wire sizes are usually given
# in area in mm^2, covered by IEC 60228, Conductors of Insulated Cables.
#
# This converts AWG to area; in general, there is no exact
# correspondence of AWG to standard metric sizes.
wiregaugeA(ga) units=[1;m^2] range=(0,) \
circlearea_d(awg(ga)); \
~awg(~circlearea_d(wiregaugeA))
wiregaA() wiregaugeA
awgA() wiregaugeA
# Next we have the SWG, the Imperial or British Standard Wire Gauge. This one
# is piecewise linear. It was used for aluminum sheets but also shows up for
# wire used in jewelry.
brwiregauge[in] \
-6 0.5 \
-5 0.464 \
-3 0.4 \
-2 0.372 \
3 0.252 \
6 0.192 \
10 0.128 \
14 0.08 \
19 0.04 \
23 0.024 \
26 0.018 \
28 0.0148 \
30 0.0124 \
39 0.0052 \
49 0.0012 \
50 0.001
swg() brwiregauge
# The following is from the Appendix to ASTM B 258
#
# For example, in U.S. gage, the standard for sheet metal is based on the
# weight of the metal, not on the thickness. 16-gage is listed as
# approximately .0625 inch thick and 40 ounces per square foot (the original
# standard was based on wrought iron at .2778 pounds per cubic inch; steel
# has almost entirely superseded wrought iron for sheet use, at .2833 pounds
# per cubic inch). Smaller numbers refer to greater thickness. There is no
# formula for converting gage to thickness or weight.
#
# It's rather unclear from the passage above whether the plate gauge values are
# therefore wrong if steel is being used. Reference [15] states that steel is
# in fact measured using this gauge (under the name Manufacturers' Standard
# Gauge) with a density of 501.84 lb/ft3 = 0.2904 lb/in3 used for steel.
# But this doesn't seem to be the correct density of steel (.2833 lb/in3 is
# closer).
#
# This gauge was established in 1893 for purposes of taxation.
# Old plate gauge for iron
plategauge[(oz/ft^2)/(480*lb/ft^3)] \
-5 300 \
1 180 \
14 50 \
16 40 \
17 36 \
20 24 \
26 12 \
31 7 \
36 4.5 \
38 4
# Manufacturers Standard Gage
stdgauge[(oz/ft^2)/(501.84*lb/ft^3)] \
-5 300 \
1 180 \
14 50 \
16 40 \
17 36 \
20 24 \
26 12 \
31 7 \
36 4.5 \
38 4
# A special gauge is used for zinc sheet metal. Notice that larger gauges
# indicate thicker sheets.
zincgauge[in] \
1 0.002 \
10 0.02 \
15 0.04 \
19 0.06 \
23 0.1 \
24 0.125 \
27 0.5 \
28 1
#
# Imperial drill bit sizes are reported in inches or in a numerical or
# letter gauge.
#
drillgauge[in] \
1 0.2280 \
2 0.2210 \
3 0.2130 \
4 0.2090 \
5 0.2055 \
6 0.2040 \
7 0.2010 \
8 0.1990 \
9 0.1960 \
10 0.1935 \
11 0.1910 \
12 0.1890 \
13 0.1850 \
14 0.1820 \
15 0.1800 \
16 0.1770 \
17 0.1730 \
18 0.1695 \
19 0.1660 \
20 0.1610 \
22 0.1570 \
23 0.1540 \
24 0.1520 \
25 0.1495 \
26 0.1470 \
27 0.1440 \
28 0.1405 \
29 0.1360 \
30 0.1285 \
31 0.1200 \
32 0.1160 \
33 0.1130 \
34 0.1110 \
35 0.1100 \
36 0.1065 \
38 0.1015 \
39 0.0995 \
40 0.0980 \
41 0.0960 \
42 0.0935 \
43 0.0890 \
44 0.0860 \
45 0.0820 \
46 0.0810 \
48 0.0760 \
51 0.0670 \
52 0.0635 \
53 0.0595 \
54 0.0550 \
55 0.0520 \
56 0.0465 \
57 0.0430 \
65 0.0350 \
66 0.0330 \
68 0.0310 \
69 0.0292 \
70 0.0280 \
71 0.0260 \
73 0.0240 \
74 0.0225 \
75 0.0210 \
76 0.0200 \
78 0.0160 \
79 0.0145 \
80 0.0135 \
88 0.0095 \
104 0.0031
drillA 0.234 in
drillB 0.238 in
drillC 0.242 in
drillD 0.246 in
drillE 0.250 in
drillF 0.257 in
drillG 0.261 in
drillH 0.266 in
drillI 0.272 in
drillJ 0.277 in
drillK 0.281 in
drillL 0.290 in
drillM 0.295 in
drillN 0.302 in
drillO 0.316 in
drillP 0.323 in
drillQ 0.332 in
drillR 0.339 in
drillS 0.348 in
drillT 0.358 in
drillU 0.368 in
drillV 0.377 in
drillW 0.386 in
drillX 0.397 in
drillY 0.404 in
drillZ 0.413 in
# Screw sizes
#
# In the USA, diameters for small wood screws, tapping screws, drive screws,
# and machine screws are reported using a gauge number. The dimensions are
# covered by ASME B 18.6.1, Wood Screws (Inch Series) and ASME B 18.6.3,
# Machine Screws, Tapping Screws, and Metallic Drive Screws (Inch Series).
# Machine screw sizes larger than 12 are reported in fractional inches; metric
# machine screws are reported as Mxx, where xx is the diameter in mm.
#
# Not all sizes apply to all screw types. The valid range for machine screws
# is 0000-12, with only even values for sizes greater than 5. The valid range
# for wood, tapping, and drive screws is 0-24, with only even values for sizes
# greater than 9.
#
# The formula below is easily inferred from tables in ASME B 18.6.1 or ASME
# B 18.6.3. The allowed range of sizes is 0000-24, but as noted above, not
# all results may be meaningful. For sizes 0000-00, use a negative value of 1
# less than the number of zeros (e.g., for #000, use -2) or the gxx or gx_0
# units as with American Wire Gauge.
screwgauge(g) units=[1;m] domain=[-3,24] range=[0.0005334,0.0094488] \
(.06 + .013 g) in ; (screwgauge/in + (-.06)) / .013
# Nominal pipe size (NPS), formerly iron pipe size (IPS) is a North American
# set of standard outside diameters (OD) for pipes. The sizes are covered by
# ASME B 36.10, Welded and Seamless Wrought Steel Pipe. The wall thickness
# (and hence the inside diameter) is determined by the schedule. The value is
# dimensionless but roughly corresponds to the outside diameter in inches.
# For smaller pipe sizes, there is only an approximate relationship between
# nominal and actual diameters: for NPS 1/8 to 12, the NPS and OD values are
# different; for NPS 14 and greater, the OD in inches is the same as the NPS.
# For example, the actual OD of an NPS 12 pipe is 12.75 inches; the OD of an
# NPS 14 pipe is 14 inches. For a given NPS, the outside diameter is
# constant; the inside diameter varies with schedule.
#
# For steel tubing, the OD is the actual size.
#
# ASME B36.10 gives OD and wall thickness; inside diameters in tables nps40,
# nps80, nps40s, and nps80s are calculated from those values
# NPS: Nominal Pipe Size
# outside diameter: all schedules
npsOD[in] \
0.125 0.405 \
0.25 0.540 \
0.375 0.675 \
0.5 0.840 \
0.75 1.050 \
1 1.315 \
1.25 1.660 \
1.5 1.900 \
2 2.375 \
2.5 2.875 \
3 3.500 \
3.5 4.000 \
4 4.500 \
5 5.563 \
6 6.625 \
8 8.625 \
10 10.750 \
12 12.750 \
14 14.000 \
16 16.000 \
18 18.000 \
20 20.000 \
24 24.000
# inside diameter: schedule 40 steel and PVC
nps40[in] \
0.125 0.269 \
0.25 0.364 \
0.375 0.493 \
0.5 0.622 \
0.75 0.824 \
1 1.049 \
1.25 1.380 \
1.5 1.610 \
2 2.067 \
2.5 2.469 \
3 3.068 \
3.5 3.548 \
4 4.026 \
5 5.047 \
6 6.065 \
8 7.981 \
10 10.020 \
12 11.938 \
14 13.124 \
16 15.000 \
18 16.876 \
20 18.812 \
24 22.626
# inside diameter: schedule 80 steel and PVC
nps80[in] \
0.125 0.215 \
0.25 0.302 \
0.375 0.423 \
0.5 0.546 \
0.75 0.742 \
1 0.957 \
1.25 1.278 \
1.5 1.500 \
2 1.939 \
2.5 2.323 \
3 2.900 \
3.5 3.364 \
4 3.826 \
5 4.813 \
6 5.761 \
8 7.625 \
10 9.564 \
12 11.376 \
14 12.500 \
16 14.314 \
18 16.126 \
20 17.938 \
24 21.564
# inside diameter: schedule 40s (stainless steel)
nps40s[in] \
0.125 0.269 \
0.25 0.364 \
0.375 0.493 \
0.5 0.622 \
0.75 0.824 \
1 1.049 \
1.25 1.380 \
1.5 1.610 \
2 2.067 \
2.5 2.469 \
3 3.068 \
3.5 3.548 \
4 4.026 \
5 5.047 \
6 6.065 \
8 7.981 \
10 10.020 \
12 12.000 \
14 13.250 \
16 15.250 \
18 17.250 \
20 19.250 \
24 23.250
# inside diameter: schedule 80s (stainless steel)
nps80s[in] \
0.125 0.215 \
0.25 0.302 \
0.375 0.423 \
0.5 0.546 \
0.75 0.742 \
1 0.957 \
1.25 1.278 \
1.5 1.500 \
2 1.939 \
2.5 2.323 \
3 2.900 \
3.5 3.364 \
4 3.826 \
5 4.813 \
6 5.761 \
8 7.625 \
10 9.750 \
12 11.750 \
14 13.000 \
16 15.000 \
18 17.000 \
20 19.000 \
24 23.000
# iron pipe size ("IPS") aliases
ipsOD() npsOD
ips40() nps40
ips80() nps80
ips40s() nps40s
ips80s() nps80s
# diamètre nominal/nominal diameter/Nennweite/NW/nominal bore/NB to NPS
# metric sizes are given in dimensionless values that very roughly correspond
# to OD in mm. The table below can be used to find pipe sizes in metric
# units, e.g., npsOD(DN(15)) = 21.336 mm
DN[1] \
6 0.125 \
8 0.25 \
10 0.375 \
15 0.5 \
20 0.75 \
25 1 \
32 1.25 \
40 1.5 \
50 2 \
65 2.5 \
80 3 \
90 3.5 \
100 4 \
115 4.5 \
125 5 \
150 6 \
200 8 \
250 10 \
300 12 \
350 14 \
400 16 \
450 18 \
500 20 \
550 22 \
600 24
NB() DN
NW() DN
# standard dimension ratio: OD to ID
# SDR = actual diameter / min wall thickness (nominally)
# copper tubing
# Copper Tube Handbook https://copper.org/applications/plumbing/cth/homepage.php
# Copper Development Association https://copper.org/
# for types K, L, and M, OD is 1/8" greater than nominal
# for ACR, OD is nominal OD
copperTubeOD[in] \
0.375 0.500 \
0.5 0.625 \
0.75 0.875 \
1 1.125 \
1.25 1.375 \
1.5 1.625 \
2 2.125 \
2.5 2.625 \
3 3.125 \
3.5 3.625 \
4 4.125 \
5 5.125 \
6 6.125 \
8 8.125 \
10 10.125 \
12 12.125
# copper tubing type K: ID
copperTypeK[in] \
0.25 0.305 \
0.375 0.402 \
0.5 0.527 \
0.625 0.652 \
0.75 0.745 \
1 0.995 \
1.25 1.245 \
1.5 1.481 \
2 1.959 \
2.5 2.435 \
3 2.907 \
3.5 3.385 \
4 3.857 \
5 4.805 \
6 5.741 \
8 7.583 \
10 9.449 \
12 11.315
# copper tubing type L: ID
copperTypeL[in] \
0.25 0.315 \
0.375 0.430 \
0.5 0.545 \
0.625 0.666 \
0.75 0.785 \
1 1.025 \
1.25 1.265 \
1.5 1.505 \
2 1.985 \
2.5 2.465 \
3 2.945 \
3.5 3.425 \
4 3.905 \
5 4.875 \
6 5.845 \
8 7.725 \
10 9.625 \
12 11.565
# copper tubing type M: ID
copperTypeM[in] \
0.375 0.450 \
0.5 0.569 \
0.75 0.811 \
1 1.055 \
1.25 1.291 \
1.5 1.527 \
2 2.009 \
2.5 2.495 \
3 2.981 \
3.5 3.459 \
4 3.935 \
5 4.907 \
6 5.881 \
8 7.785 \
10 9.701 \
12 11.617
# copper tubing: air conditioning and refrigeration: ID
# ID is the same as for type L of the same actual OD
copperTypeACR[in] \
0.25 0.200 \
0.375 0.315 \
0.5 0.430 \
0.625 0.545 \
0.75 0.666 \
0.875 0.785 \
1.125 1.025 \
1.375 1.265 \
1.625 1.505 \
2.125 1.985 \
2.625 2.465 \
3.125 2.945 \
3.625 3.425 \
4.125 3.905
copperOD() copperTubeOD
copperK() copperTypeK
copperL() copperTypeL
copperM() copperTypeM
copperACR() copperTypeACR
#
# Abrasive grit size
#
# Standards governing abrasive grit sizes are complicated, specifying
# fractions of particles that are passed or retained by different mesh
# sizes. As a result, it is not possible to make precise comparisons
# of different grit standards. The tables below allow the
# determination of rough equivlants by using median particle size.
#
# Standards in the USA are determined by the Unified Abrasives
# Manufacturers' Association (UAMA), which resulted from the merger of
# several previous organizations. One of the old organizations was
# CAMI (Coated Abrasives Manufacturers' Institute).
#
# UAMA has a web page with plots showing abrasive particle ranges for
# various different grits and comparisons between standards.
#
# https://uama.org/abrasives-101/
#
# Abrasives are grouped into "bonded" abrasives for use with grinding
# wheels and "coated" abrasives for sandpapers and abrasive films.
# The industry uses different grit standards for these two
# categories.
#
# Another division is between "macrogrits", grits below 240 and
# "microgrits", which are above 240. Standards differ, as do methods
# for determining particle size. In the USA, ANSI B74.12 is the
# standard governing macrogrits. ANSI B74.10 covers bonded microgrit
# abrasives, and ANSI B74.18 covers coated microgrit abrasives. It
# appears that the coated standard is identical to the bonded standard
# for grits up through 600 but then diverges significantly.
#
# European grit sizes are determined by the Federation of European
# Producers of Abrasives. http://www.fepa-abrasives.org
#
# They give two standards, the "F" grit for bonded abrasives and the
# "P" grit for coated abrasives. This data is taken directly from
# their web page.
# FEPA P grit for coated abrasives is commonly seen on sandpaper in
# the USA where the paper will be marked P600, for example. FEPA P
# grits are said to be more tightly constrained than comparable ANSI
# grits so that the particles are more uniform in size and hence give
# a better finish.
grit_P[micron] \
12 1815 \
16 1324 \
20 1000 \
24 764 \
30 642 \
36 538 \
40 425 \
50 336 \
60 269 \
80 201 \
100 162 \
120 125 \
150 100 \
180 82 \
220 68 \
240 58.5 \
280 52.2 \
320 46.2 \
360 40.5 \
400 35 \
500 30.2 \
600 25.8 \
800 21.8 \
1000 18.3 \
1200 15.3 \
1500 12.6 \
2000 10.3 \
2500 8.4
# The F grit is the European standard for bonded abrasives such as
# grinding wheels
grit_F[micron] \
4 4890 \
5 4125 \
6 3460 \
7 2900 \
8 2460 \
10 2085 \
12 1765 \
14 1470 \
16 1230 \
20 1040 \
22 885 \
24 745 \
30 625 \
36 525 \
40 438 \
46 370 \
54 310 \
60 260 \
70 218 \
80 185 \
90 154 \
100 129 \
120 109 \
150 82 \
180 69 \
220 58 \
230 53 \
240 44.5 \
280 36.5 \
320 29.2 \
360 22.8 \
400 17.3 \
500 12.8 \
600 9.3 \
800 6.5 \
1000 4.5 \
1200 3 \
1500 2.0 \
2000 1.2
# According to the UAMA web page, the ANSI bonded and ANSI coated standards
# are identical to FEPA F in the macrogrit range (under 240 grit), so these
# values are taken from the FEPA F table. The values for 240 and above are
# from the UAMA web site and represent the average of the "d50" range
# endpoints listed there.
ansibonded[micron] \
4 4890 \
5 4125 \
6 3460 \
7 2900 \
8 2460 \
10 2085 \
12 1765 \
14 1470 \
16 1230 \
20 1040 \
22 885 \
24 745 \
30 625 \
36 525 \
40 438 \
46 370 \
54 310 \
60 260 \
70 218 \
80 185 \
90 154 \
100 129 \
120 109 \
150 82 \
180 69 \
220 58 \
240 50 \
280 39.5 \
320 29.5 \
360 23 \
400 18.25 \
500 13.9 \
600 10.55 \
800 7.65 \
1000 5.8 \
1200 3.8
grit_ansibonded() ansibonded
# Like the bonded grit, the coated macrogrits below 240 are taken from the
# FEPA F table. Data above this is from the UAMA site. Note that the coated
# and bonded standards are evidently the same from 240 up to 600 grit, but
# starting at 800 grit, the coated standard diverges. The data from UAMA show
# that 800 grit coated has an average size slightly larger than the average
# size of 600 grit coated/bonded. However, the 800 grit has a significantly
# smaller particle size variation.
#
# Because of this non-monotonicity from 600 grit to 800 grit this definition
# produces a warning about the lack of a unique inverse.
ansicoated[micron] noerror \
4 4890 \
5 4125 \
6 3460 \
7 2900 \
8 2460 \
10 2085 \
12 1765 \
14 1470 \
16 1230 \
20 1040 \
22 885 \
24 745 \
30 625 \
36 525 \
40 438 \
46 370 \
54 310 \
60 260 \
70 218 \
80 185 \
90 154 \
100 129 \
120 109 \
150 82 \
180 69 \
220 58 \
240 50 \
280 39.5 \
320 29.5 \
360 23 \
400 18.25 \
500 13.9 \
600 10.55 \
800 11.5 \
1000 9.5 \
2000 7.2 \
2500 5.5 \
3000 4 \
4000 3 \
6000 2 \
8000 1.2
grit_ansicoated() ansicoated
#
# Is this correct? This is the JIS Japanese standard used on waterstones
#
jisgrit[micron] \
150 75 \
180 63 \
220 53 \
280 48 \
320 40 \
360 35 \
400 30 \
600 20 \
700 17 \
800 14 \
1000 11.5 \
1200 9.5 \
1500 8 \
2000 6.7 \
2500 5.5 \
3000 4 \
4000 3 \
6000 2 \
8000 1.2
# The "Finishing Scale" marked with an A (e.g. A75). This information
# is from the web page of the sand paper manufacturer Klingspor
# https://www.klingspor.com/ctemplate1.aspx?page=default/html/gritGradingSystems_en-US.html
#
# I have no information about what this scale is used for.
grit_A[micron]\
16 15.3 \
25 21.8 \
30 23.6 \
35 25.75 \
45 35 \
60 46.2 \
65 53.5 \
75 58.5 \
90 65 \
110 78 \
130 93 \
160 127 \
200 156
#
# Grits for DMT brand diamond sharpening stones from
# https://www.dmtsharp.com/resources/dmt-catalog-product-information.html
# "DMT Diamond Grits" PDF download
dmtxxcoarse 120 micron # 120 mesh
dmtsilver dmtxxcoarse
dmtxx dmtxxcoarse
dmtxcoarse 60 micron # 220 mesh
dmtx dmtxcoarse
dmtblack dmtxcoarse
dmtcoarse 45 micron # 325 mesh
dmtc dmtcoarse
dmtblue dmtcoarse
dmtfine 25 micron # 600 mesh
dmtred dmtfine
dmtf dmtfine
dmtefine 9 micron # 1200 mesh
dmte dmtefine
dmtgreen dmtefine
dmtceramic 7 micron # 2200 mesh
dmtcer dmtceramic
dmtwhite dmtceramic
dmteefine 3 micron # 8000 mesh
dmttan dmteefine
dmtee dmteefine
#
# The following values come from a page in the Norton Stones catalog,
# available at their web page, http://www.nortonstones.com.
#
hardtranslucentarkansas 6 micron # Natural novaculite (silicon quartz)
softarkansas 22 micron # stones
extrafineindia 22 micron # India stones are Norton's manufactured
fineindia 35 micron # aluminum oxide product
mediumindia 53.5 micron
coarseindia 97 micron
finecrystolon 45 micron # Crystolon stones are Norton's
mediumcrystalon 78 micron # manufactured silicon carbide product
coarsecrystalon 127 micron
# The following are not from the Norton catalog
hardblackarkansas 6 micron
hardwhitearkansas 11 micron
washita 35 micron
#
# Mesh systems for measuring particle sizes by sifting through a wire
# mesh or sieve
#
# The Tyler system and US Sieve system are based on four steps for
# each factor of 2 change in the size, so each size is 2^1|4 different
# from the adjacent sizes. Unfortunately, the mesh numbers are
# arbitrary, so the sizes cannot be expressed with a functional form.
# Various references round the values differently. The mesh numbers
# are supposed to correspond to the number of holes per inch, but this
# correspondence is only approximate because it doesn't include the
# wire size of the mesh.
# The Tyler Mesh system was apparently introduced by the WS Tyler
# company, but it appears that they no longer use it. They follow the
# ASTM E11 standard.
meshtyler[micron] \
2.5 8000 \
3 6727 \
3.5 5657 \
4 4757 \
5 4000 \
6 3364 \
7 2828 \
8 2378 \
9 2000 \
10 1682 \
12 1414 \
14 1189 \
16 1000 \
20 841 \
24 707 \
28 595 \
32 500 \
35 420 \
42 354 \
48 297 \
60 250 \
65 210 \
80 177 \
100 149 \
115 125 \
150 105 \
170 88 \
200 74 \
250 63 \
270 53 \
325 44 \
400 37
# US Sieve size, ASTM E11
#
# The WS Tyler company prints the list from ASTM E11 in
# A Calculator for ASTM E11 Standard Sieve Designations
# https://blog.wstyler.com/particle-analysis/astm-e11-standard-designations
sieve[micron] \
3.5 5600 \
4 4750 \
5 4000 \
6 3350 \
7 2800 \
8 2360 \
10 2000 \
12 1700 \
14 1400 \
16 1180 \
18 1000 \
20 850 \
25 710 \
30 600 \
35 500 \
40 425 \
45 355 \
50 300 \
60 250 \
70 212 \
80 180 \
100 150 \
120 125 \
140 106 \
170 90 \
200 75 \
230 63 \
270 53 \
325 45 \
400 38 \
450 32 \
500 25 \
625 20 # These last two values are not in the standard series
# but were included in the ASTM standard because they
meshUS() sieve # were in common usage.
# British Mesh size, BS 410: 1986
# This system appears to correspond to the Tyler and US system, but
# with different mesh numbers.
#
# http://www.panadyne.com/technical/panadyne_international_sieve_chart.pdf
#
meshbritish[micron] \
3 5657 \
3.5 4757 \
4 4000 \
5 3364 \
6 2828 \
7 2378 \
8 2000 \
10 1682 \
12 1414 \
14 1189 \
16 1000 \
18 841 \
22 707 \
25 595 \
30 500 \
36 420 \
44 354 \
52 297 \
60 250 \
72 210 \
85 177 \
100 149 \
120 125 \
150 105 \
170 88 \
200 74 \
240 63 \
300 53 \
350 44 \
400 37
# French system, AFNOR NFX11-501: 1970
# The system appears to be based on size doubling every 3 mesh
# numbers, though the values have been aggressively rounded.
# It's not clear if the unrounded values would be considered
# incorrect, so this is given as a table rather than a function.
# Functional form:
# meshtamis(mesh) units=[1;m] 5000 2^(1|3 (mesh-38)) micron
#
# http://www.panadyne.com/technical/panadyne_international_sieve_chart.pdf
meshtamis[micron] \
17 40 \
18 50 \
19 63 \
20 80 \
21 100 \
22 125 \
23 160 \
24 200 \
25 250 \
26 315 \
27 400 \
28 500 \
29 630 \
30 800 \
31 1000 \
32 1250 \
33 1600 \
34 2000 \
35 2500 \
36 3150 \
37 4000 \
38 5000
#
# Ring size. All ring sizes are given as the circumference of the ring.
#
# USA ring sizes. Several slightly different definitions seem to be in
# circulation. According to [15], the interior diameter of size n ring in
# inches is 0.32 n + 0.458 for n ranging from 3 to 13.5 by steps of 0.5. The
# size 2 ring is inconsistently 0.538in and no 2.5 size is listed.
#
# However, other sources list 0.455 + 0.0326 n and 0.4525 + 0.0324 n as the
# diameter and list no special case for size 2. (Or alternatively they are
# 1.43 + .102 n and 1.4216+.1018 n for measuring circumference in inches.) One
# reference claimed that the original system was that each size was 1|10 inch
# circumference, but that source doesn't have an explanation for the modern
# system which is somewhat different.
ringsize(n) units=[1;in] domain=[2,) range=[1.6252,) \
(1.4216+.1018 n) in ; (ringsize/in + (-1.4216))/.1018
# Old practice in the UK measured rings using the "Wheatsheaf gauge" with sizes
# specified alphabetically and based on the ring inside diameter in steps of
# 1|64 inch. This system was replaced in 1987 by British Standard 6820 which
# specifies sizes based on circumference. Each size is 1.25 mm different from
# the preceding size. The baseline is size C which is 40 mm circumference.
# The new sizes are close to the old ones. Sometimes it's necessary to go
# beyond size Z to Z+1, Z+2, etc.
sizeAring 37.50 mm
sizeBring 38.75 mm
sizeCring 40.00 mm
sizeDring 41.25 mm
sizeEring 42.50 mm
sizeFring 43.75 mm
sizeGring 45.00 mm
sizeHring 46.25 mm
sizeIring 47.50 mm
sizeJring 48.75 mm
sizeKring 50.00 mm
sizeLring 51.25 mm
sizeMring 52.50 mm
sizeNring 53.75 mm
sizeOring 55.00 mm
sizePring 56.25 mm
sizeQring 57.50 mm
sizeRring 58.75 mm
sizeSring 60.00 mm
sizeTring 61.25 mm
sizeUring 62.50 mm
sizeVring 63.75 mm
sizeWring 65.00 mm
sizeXring 66.25 mm
sizeYring 67.50 mm
sizeZring 68.75 mm
# Japanese sizes start with size 1 at a 13mm inside diameter and each size is
# 1|3 mm larger in diameter than the previous one. They are multiplied by pi
# to give circumference.
jpringsize(n) units=[1;mm] domain=[1,) range=[0.040840704,) \
(38|3 + n/3) pi mm ; 3 jpringsize/ pi mm + (-38)
# The European ring sizes are the length of the circumference in mm minus 40.
euringsize(n) units=[1;mm] (n+40) mm ; euringsize/mm + (-40)
#
# Abbreviations
#
mph mile/hr
brmpg mile/brgallon
usmpg mile/usgallon
mpg mile/gal
kph km/hr
fL footlambert
fpm ft/min
fps ft/s
rpm rev/min
rps rev/sec
mi mile
smi mile
nmi nauticalmile
mbh 1e3 btu/hour
mcm 1e3 circularmil
ipy inch/year # used for corrosion rates
ccf 100 ft^3 # used for selling water [18]
Mcf 1000 ft^3 # not million cubic feet [18]
kp kilopond
kpm kp meter
Wh W hour
hph hp hour
plf lb / foot # pounds per linear foot
#
# Compatibility units with Unix version
#
pa Pa
ev eV
hg Hg
oe Oe
mh mH
rd rod
pf pF
gr grain
nt N
hz Hz
hd hogshead
dry drygallon/gallon
nmile nauticalmile
beV GeV
bev beV
coul C
#
# Radioactivity units
#
event !dimensionless
becquerel event /s # Activity of radioactive source
Bq becquerel #
curie 3.7e10 Bq # Defined in 1910 as the radioactivity
Ci curie # emitted by the amount of radon that is
# in equilibrium with 1 gram of radium.
rutherford 1e6 Bq #
RADIATION_DOSE gray
gray J/kg # Absorbed dose of radiation
Gy gray #
rad 1e-2 Gy # From Radiation Absorbed Dose
rep 8.38 mGy # Roentgen Equivalent Physical, the amount
# of radiation which , absorbed in the
# body, would liberate the same amount
# of energy as 1 roentgen of X rays
# would, or 97 ergs.
sievert J/kg # Dose equivalent: dosage that has the
Sv sievert # same effect on human tissues as 200
rem 1e-2 Sv # keV X-rays. Different types of
# radiation are weighted by the
# Relative Biological Effectiveness
# (RBE).
#
# Radiation type RBE
# X-ray, gamma ray 1
# beta rays, > 1 MeV 1
# beta rays, < 1 MeV 1.08
# neutrons, < 1 MeV 4-5
# neutrons, 1-10 MeV 10
# protons, 1 MeV 8.5
# protons, .1 MeV 10
# alpha, 5 MeV 15
# alpha, 1 MeV 20
#
# The energies are the kinetic energy
# of the particles. Slower particles
# interact more, so they are more
# effective ionizers, and hence have
# higher RBE values.
#
# rem stands for Roentgen Equivalent
# Mammal
banana_dose 0.1e-6 sievert # Informal measure of the dose due to
# eating one average sized banana
roentgen 2.58e-4 C / kg # Ionizing radiation that produces
# 1 statcoulomb of charge in 1 cc of
# dry air at stp.
rontgen roentgen # Sometimes it appears spelled this way
sievertunit 8.38 rontgen # Unit of gamma ray dose delivered in one
# hour at a distance of 1 cm from a
# point source of 1 mg of radium
# enclosed in platinum .5 mm thick.
eman 1e-7 Ci/m^3 # radioactive concentration
mache 3.7e-7 Ci/m^3
#
# Atomic weights. The atomic weight of an element is the ratio of the mass of
# a mole of the element to 1|12 of a mole of Carbon 12. For each element, we
# list the atomic weights of all of the isotopes. The Standard Atomic Weights
# apply to the elements in the isotopic composition that occurs naturally on
# Earth. These are computed values based on the isotopic distribution, and
# may vary for specific samples. Elements which do not occur naturally do
# not have Standard Atomic Weights. For these elements, if data on the most
# stable isotope is available, is given. Otherwise, the user must specify the
# desired isotope.
!include elements.units
# Density of the elements
#
# Note some elements occur in multiple forms (allotropes) with different
# densities, and they are accordingly listed multiple times.
# Density of gas phase elements at STP
hydrogendensity 0.08988 g/l
heliumdensity 0.1786 g/l
neondensity 0.9002 g/l
nitrogendensity 1.2506 g/l
oxygendensity 1.429 g/l
fluorinedensity 1.696 g/l
argondensity 1.784 g/l
chlorinedensity 3.2 g/l
kryptondensity 3.749 g/l
xenondensity 5.894 g/l
radondensity 9.73 g/l
# Density of liquid phase elements near room temperature
brominedensity 3.1028 g/cm^3
mercurydensity 13.534 g/cm^3
# Density of solid elements near room temperature
lithiumdensity 0.534 g/cm^3
potassiumdensity 0.862 g/cm^3
sodiumdensity 0.968 g/cm^3
rubidiumdensity 1.532 g/cm^3
calciumdensity 1.55 g/cm^3
magnesiumdensity 1.738 g/cm^3
phosphorus_white_density 1.823 g/cm^3
berylliumdensity 1.85 g/cm^3
sulfur_gamma_density 1.92 g/cm^3
cesiumdensity 1.93 g/cm^3
carbon_amorphous_density 1.95 g/cm^3 # average value
sulfur_betadensity 1.96 g/cm^3
sulfur_alpha_density 2.07 g/cm^3
carbon_graphite_density 2.267 g/cm^3
phosphorus_red_density 2.27 g/cm^3 # average value
silicondensity 2.3290 g/cm^3
phosphorus_violet_density 2.36 g/cm^3
borondensity 2.37 g/cm^3
strontiumdensity 2.64 g/cm^3
phosphorus_black_density 2.69 g/cm^3
aluminumdensity 2.7 g/cm^3
bariumdensity 3.51 g/cm^3
carbon_diamond_density 3.515 g/cm^3
scandiumdensity 3.985 g/cm^3
selenium_vitreous_density 4.28 g/cm^3
selenium_alpha_density 4.39 g/cm^3
titaniumdensity 4.406 g/cm^3
yttriumdensity 4.472 g/cm^3
selenium_gray_density 4.81 g/cm^3
iodinedensity 4.933 g/cm^3
europiumdensity 5.264 g/cm^3
germaniumdensity 5.323 g/cm^3
radiumdensity 5.5 g/cm^3
arsenicdensity 5.727 g/cm^3
tin_alpha_density 5.769 g/cm^3
galliumdensity 5.91 g/cm^3
vanadiumdensity 6.11 g/cm^3
lanthanumdensity 6.162 g/cm^3
telluriumdensity 6.24 g/cm^3
zirconiumdensity 6.52 g/cm^3
antimonydensity 6.697 g/cm^3
ceriumdensity 6.77 g/cm^3
praseodymiumdensity 6.77 g/cm^3
ytterbiumdensity 6.9 g/cm^3
neodymiumdensity 7.01 g/cm^3
zincdensity 7.14 g/cm^3
chromiumdensity 7.19 g/cm^3
manganesedensity 7.21 g/cm^3
promethiumdensity 7.26 g/cm^3
tin_beta_density 7.265 g/cm^3
indiumdensity 7.31 g/cm^3
samariumdensity 7.52 g/cm^3
irondensity 7.874 g/cm^3
gadoliniumdensity 7.9 g/cm^3
terbiumdensity 8.23 g/cm^3
dysprosiumdensity 8.54 g/cm^3
niobiumdensity 8.57 g/cm^3
cadmiumdensity 8.65 g/cm^3
holmiumdensity 8.79 g/cm^3
cobaltdensity 8.9 g/cm^3
nickeldensity 8.908 g/cm^3
erbiumdensity 9.066 g/cm^3
polonium_alpha_density 9.196 g/cm^3
thuliumdensity 9.32 g/cm^3
polonium_beta_density 9.398 g/cm^3
bismuthdensity 9.78 g/cm^3
lutetiumdensity 9.841 g/cm^3
actiniumdensity 10 g/cm^3
molybdenumdensity 10.28 g/cm^3
silverdensity 10.49 g/cm^3
technetiumdensity 11 g/cm^3
leaddensity 11.34 g/cm^3
thoriumdensity 11.7 g/cm^3
thalliumdensity 11.85 g/cm^3
americiumdensity 12 g/cm^3
palladiumdensity 12.023 g/cm^3
rhodiumdensity 12.41 g/cm^3
rutheniumdensity 12.45 g/cm^3
berkelium_beta_density 13.25 g/cm^3
hafniumdensity 13.31 g/cm^3
curiumdensity 13.51 g/cm^3
berkelium_alphadensity 14.78 g/cm^3
californiumdensity 15.1 g/cm^3
protactiniumdensity 15.37 g/cm^3
tantalumdensity 16.69 g/cm^3
uraniumdensity 19.1 g/cm^3
tungstendensity 19.3 g/cm^3
golddensity 19.30 g/cm^3
plutoniumdensity 19.816 g/cm^3
neptuniumdensity 20.45 g/cm^3 # alpha form, only one at room temp
rheniumdensity 21.02 g/cm^3
platinumdensity 21.45 g/cm^3
iridiumdensity 22.56 g/cm^3
osmiumdensity 22.59 g/cm^3
# A few alternate names
tin_gray tin_alpha_density
tin_white tin_beta_density
graphitedensity carbon_graphite_density
diamonddensity carbon_diamond_density
# Predicted density of elements that have not been made in sufficient
# quantities for measurement.
franciumdensity 2.48 g/cm^3 # liquid, predicted melting point 8 degC
astatinedensity 6.35 g/cm^3
einsteiniumdensity 8.84 g/cm^3
fermiumdensity 9.7 g/cm^3
nobeliumdensity 9.9 g/cm^3
mendeleviumdensity 10.3 g/cm^3
lawrenciumdensity 16 g/cm^3
rutherfordiumdensity 23.2 g/cm^3
roentgeniumdensity 28.7 g/cm^3
dubniumdensity 29.3 g/cm^3
darmstadtiumdensity 34.8 g/cm^3
seaborgiumdensity 35 g/cm^3
bohriumdensity 37.1 g/cm^3
meitneriumdensity 37.4 g/cm^3
hassiumdensity 41 g/cm^3
#
# population units
#
people 1
person people
death people
capita people
percapita per capita
# TGM dozen based unit system listed on the "dozenal" forum
# http://www.dozenalsociety.org.uk/apps/tgm.htm. These units are
# proposed as an allegedly more rational alternative to the SI system.
Tim 12^-4 hour # Time
Grafut gravity Tim^2 # Length based on gravity
Surf Grafut^2 # area
Volm Grafut^3 # volume
Vlos Grafut/Tim # speed
Denz Maz/Volm # density
Mag Maz gravity # force
Maz Volm kg / oldliter # mass based on water
# Abbreviations
# Tm Tim # Conflicts with Tm = Terameter
Gf Grafut
Sf Surf
Vm Volm
Vl Vlos
Mz Maz
Dz Denz
# Dozen based unit prefixes
Zena- 12
Duna- 12^2
Trina- 12^3
Quedra- 12^4
Quena- 12^5
Hesa- 12^6
Seva- 12^7
Aka- 12^8
Neena- 12^9
Dexa- 12^10
Lefa- 12^11
Zennila- 12^12
Zeni- 12^-1
Duni- 12^-2
Trini- 12^-3
Quedri- 12^-4
Queni- 12^-5
Hesi- 12^-6
Sevi- 12^-7
Aki- 12^-8
Neeni- 12^-9
Dexi- 12^-10
Lefi- 12^-11
Zennili- 12^-12
#
# Traditional Japanese units (shakkanhou)
#
# The traditional system of weights and measures is called shakkanhou from the
# shaku and the ken. Japan accepted SI units in 1891 and legalized conversions
# to the traditional system. In 1909 the inch-pound system was also legalized,
# so Japan had three legally approved systems. A change to the metric system
# started in 1921 but there was a lot of resistance. The Measurement Law of
# October 1999 prohibits sales in anything but SI units. However, the old
# units still live on in construction and as the basis for paper sizes of books
# and tools used for handicrafts.
#
# Note that units below use the Hepburn romanization system. Some other
# systems would render "mou", "jou", and "chou" as "mo", "jo" and "cho".
#
#
# http://hiramatu-hifuka.com/onyak/onyindx.html
# Japanese Proportions. These are still in everyday use. They also
# get used as units to represent the proportion of the standard unit.
wari_proportion 1|10
wari wari_proportion
bu_proportion 1|100 # The character bu can also be read fun or bun
# but usually "bu" is used for units.
rin_proportion 1|1000
mou_proportion 1|10000
# Japanese Length Measures
#
# The length system is called kanejaku or
# square and originated in China. It was
# adopted as Japan's official measure in 701
# by the Taiho Code. This system is still in
# common use in architecture and clothing.
shaku 1|3.3 m
mou 1|10000 shaku
rin 1|1000 shaku
bu_distance 1|100 shaku
sun 1|10 shaku
jou_distance 10 shaku
jou jou_distance
kanejakusun sun # Alias to emphasize architectural name
kanejaku shaku
kanejakujou jou
# http://en.wikipedia.org/wiki/Taiwanese_units_of_measurement
taichi shaku # http://zh.wikipedia.org/wiki/台尺
taicun sun # http://zh.wikipedia.org/wiki/台制
!utf8
台尺 taichi # via Hanyu Pinyin romanizations
台寸 taicun
!endutf8
# In context of clothing, shaku is different from architecture
kujirajaku 10|8 shaku
kujirajakusun 1|10 kujirajaku
kujirajakubu 1|100 kujirajaku
kujirajakujou 10 kujirajaku
tan_distance 3 kujirajakujou
ken 6 shaku # Also sometimes 6.3, 6.5, or 6.6
# http://www.homarewood.co.jp/syakusun.htm
# mostly unused
chou_distance 60 ken
chou chou_distance
ri 36 chou
# Japanese Area Measures
# Tsubo is still used for land size, though the others are more
# recognized by their homonyms in the other measurements.
gou_area 1|10 tsubo
tsubo 36 shaku^2 # Size of two tatami = ken^2 ??
se 30 tsubo
tan_area 10 se
chou_area 10 tan_area
# http://en.wikipedia.org/wiki/Taiwanese_units_of_measurement
ping tsubo # http://zh.wikipedia.org/wiki/坪
jia 2934 ping # http://zh.wikipedia.org/wiki/甲_(单位)
fen 1|10 jia # http://zh.wikipedia.org/wiki/分
fen_area 1|10 jia # Protection against future collisions
!utf8
坪 ping # via Hanyu Pinyin romanizations
甲 jia
分 fen
分地 fen_area # Protection against future collisions
!endutf8
# Japanese architecture is based on a "standard" size of tatami mat.
# Room sizes today are given in number of tatami, and this number
# determines the spacing between colums and hence sizes of sliding
# doors and paper screens. However, every region has its own slightly
# different tatami size. Edoma, used in and around Tokyo and
# Hokkaido, is becoming a nationwide standard. Kyouma is used around
# Kyoto, Osaka and Kyuushu, and Chuukyouma is used around Nagoya.
# Note that the tatami all have the aspect ratio 2:1 so that the mats
# can tile the room with some of them turned 90 degrees.
#
# http://www.moon2.net/tatami/infotatami/structure.html
edoma (5.8*2.9) shaku^2
kyouma (6.3*3.15) shaku^2
chuukyouma (6*3) shaku^2
jou_area edoma
tatami jou_area
# Japanese Volume Measures
# The "shou" is still used for such things as alcohol and seasonings.
# Large quantities of paint are still purchased in terms of "to".
shaku_volume 1|10 gou_volume
gou_volume 1|10 shou
gou gou_volume
shou (4.9*4.9*2.7) sun^3 # The character shou which is
# the same as masu refers to a
# rectangular wooden cup used to
# measure liquids and cereal.
# Sake is sometimes served in a masu
# Note that it happens to be
# EXACTLY 7^4/11^3 liters.
to 10 shou
koku 10 to # No longer used; historically a measure of rice
# Japanese Weight Measures
#
# https://web.archive.org/web/20040927115452/http://wyoming.hp.infoseek.co.jp/zatugaku/zamoney.html
# https://en.wikipedia.org/wiki/Japanese_units_of_measurement
# Not really used anymore.
rin_weight 1|10 bu_weight
bu_weight 1|10 monme
fun 1|10 monme
monme momme
kin 160 monme
kan 1000 monme
kwan kan # This was the old pronunciation of the unit.
# The old spelling persisted a few centuries
# longer and was not changed until around
# 1950.
# http://en.wikipedia.org/wiki/Taiwanese_units_of_measurement
# says: "Volume measure in Taiwan is largely metric".
taijin kin # http://zh.wikipedia.org/wiki/台斤
tailiang 10 monme # http://zh.wikipedia.org/wiki/台斤
taiqian monme # http://zh.wikipedia.org/wiki/台制
!utf8
台斤 taijin # via Hanyu Pinyin romanizations
台兩 tailiang
台錢 taiqian
!endutf8
#
# Australian unit
#
australiasquare (10 ft)^2 # Used for house area
#
# A few German units as currently in use.
#
zentner 50 kg
doppelzentner 2 zentner
pfund 500 g
# The klafter, which was used in central Europe, was derived from the span of
# outstretched arms.
#
# https://en.wikipedia.org/wiki/Obsolete_Austrian_units_of_measurement
# https://www.llv.li/files/abi/klafter-m2-en.pdf
austriaklafter 1.89648384 m # Exact definition, 23 July 1871
austriafoot 1|6 austriaklafter
prussiaklafter 1.88 m
prussiafoot 1|6 prussiaklafter
bavariaklafter 1.751155 m
bavariafoot 1|6 bavariaklafter
hesseklafter 2.5 m
hessefoot 1|6 hesseklafter
switzerlandklafter metricklafter
switzerlandfoot 1|6 switzerlandklafter
swissklafter switzerlandklafter
swissfoot 1|6 swissklafter
metricklafter 1.8 m
austriayoke 8 austriaklafter * 200 austriaklafter
liechtensteinsquareklafter 3.596652 m^2 # Used until 2017 to measure land area
liechtensteinklafter sqrt(liechtensteinsquareklafter)
# The klafter was also used to measure volume of wood, generally being a stack
# of wood one klafter wide, one klafter long, with logs 3 feet (half a klafter)
# in length
prussiawoodklafter 0.5 prussiaklafter^3
austriawoodklafter 0.5 austriaklafter^3
festmeter m^3 # modern measure of wood, solid cube
raummeter 0.7 festmeter # Air space between the logs, stacked
schuettraummeter 0.65 raummeter # A cubic meter volume of split and cut
# firewood in a loose, unordered
# pile, not stacked. This is called
# "tipped".
!utf8
schüttraummeter schuettraummeter
!endutf8
#
# Swedish (Sweden) pre-metric units of 1739.
# The metric system was adopted in 1878.
# https://sv.wikipedia.org/wiki/Verkm%C3%A5tt
#
verklinje 2.0618125 mm
verktum 12 verklinje
kvarter 6 verktum
fot 2 kvarter
aln 2 fot
famn 3 aln
#
# Some traditional Russian measures
#
# If you would like to help expand this section and understand
# cyrillic transliteration, let me know. These measures are meant to
# reflect common usage, e.g. in translated literature.
#
dessiatine 2400 sazhen^2 # Land measure
dessjatine dessiatine
funt 409.51718 grams # similar to pound
zolotnik 1|96 funt # used for precious metal measure
pood 40 funt # common in agricultural measure
arshin (2 + 1|3) feet
sazhen 3 arshin # analogous to fathom
verst 500 sazhen # of similar use to mile
versta verst
borderverst 1000 sazhen
russianmile 7 verst
#
# Old French distance measures, from French Weights and Measures
# Before the Revolution by Zupko
#
frenchfoot 144|443.296 m # pied de roi, the standard of Paris.
pied frenchfoot # Half of the hashimicubit,
frenchfeet frenchfoot # instituted by Charlemagne.
frenchinch 1|12 frenchfoot # This exact definition comes from
frenchthumb frenchinch # a law passed on 10 Dec 1799 which
pouce frenchthumb # fixed the meter at
# 3 frenchfeet + 11.296 lignes.
frenchline 1|12 frenchinch # This is supposed to be the size
ligne frenchline # of the average barleycorn
frenchpoint 1|12 frenchline
toise 6 frenchfeet
arpent 180^2 pied^2 # The arpent is 100 square perches,
# but the perche seems to vary a lot
# and can be 18 feet, 20 feet, or 22
# feet. This measure was described
# as being in common use in Canada in
# 1934 (Websters 2nd). The value
# given here is the Paris standard
# arpent.
frenchgrain 1|18827.15 kg # Weight of a wheat grain, hence
# smaller than the British grain.
frenchpound 9216 frenchgrain
#
# Before the Imperial Weights and Measures Act of 1824, various different
# weights and measures were in use in different places.
#
# Scots linear measure
scotsinch 1.00540054 UKinch
scotslink 1|100 scotschain
scotsfoot 12 scotsinch
scotsfeet scotsfoot
scotsell 37 scotsinch
scotsfall 6 scotsell
scotschain 4 scotsfall
scotsfurlong 10 scotschain
scotsmile 8 scotsfurlong
# Scots area measure
scotsrood 40 scotsfall^2
scotsacre 4 scotsrood
# Irish linear measure
irishinch UKinch
irishpalm 3 irishinch
irishspan 3 irishpalm
irishfoot 12 irishinch
irishfeet irishfoot
irishcubit 18 irishinch
irishyard 3 irishfeet
irishpace 5 irishfeet
irishfathom 6 irishfeet
irishpole 7 irishyard # Only these values
irishperch irishpole # are different from
irishchain 4 irishperch # the British Imperial
irishlink 1|100 irishchain # or English values for
irishfurlong 10 irishchain # these lengths.
irishmile 8 irishfurlong #
# Irish area measure
irishrood 40 irishpole^2
irishacre 4 irishrood
# English wine capacity measures (Winchester measures)
winepint 1|2 winequart
winequart 1|4 winegallon
winegallon 231 UKinch^3 # Sometimes called the Winchester Wine Gallon,
# it was legalized in 1707 by Queen Anne, and
# given the definition of 231 cubic inches. It
# had been in use for a while as 8 pounds of wine
# using a merchant's pound, but the definition of
# the merchant's pound had become uncertain. A
# pound of 15 tower ounces (6750 grains) had been
# common, but then a pound of 15 troy ounces
# (7200 grains) gained popularity. Because of
# the switch in the value of the merchants pound,
# the size of the wine gallon was uncertain in
# the market, hence the official act in 1707.
# The act allowed that a six inch tall cylinder
# with a 7 inch diameter was a lawful wine
# gallon. (This comes out to 230.9 in^3.)
# Note also that in Britain a legal conversion
# was established to the 1824 Imperial gallon
# then taken as 277.274 in^3 so that the wine
# gallon was 0.8331 imperial gallons. This is
# 231.1 cubic inches (using the international
# inch).
winerundlet 18 winegallon
winebarrel 31.5 winegallon
winetierce 42 winegallon
winehogshead 2 winebarrel
winepuncheon 2 winetierce
winebutt 2 winehogshead
winepipe winebutt
winetun 2 winebutt
# English beer and ale measures used 1803-1824 and used for beer before 1688
beerpint 1|2 beerquart
beerquart 1|4 beergallon
beergallon 282 UKinch^3
beerbarrel 36 beergallon
beerhogshead 1.5 beerbarrel
# English ale measures used from 1688-1803 for both ale and beer
alepint 1|2 alequart
alequart 1|4 alegallon
alegallon beergallon
alebarrel 34 alegallon
alehogshead 1.5 alebarrel
# Scots capacity measure
scotsgill 1|4 mutchkin
mutchkin 1|2 choppin
choppin 1|2 scotspint
scotspint 1|2 scotsquart
scotsquart 1|4 scotsgallon
scotsgallon 827.232 UKinch^3
scotsbarrel 8 scotsgallon
jug scotspint
# Scots dry capacity measure
scotswheatlippy 137.333 UKinch^3 # Also used for peas, beans, rye, salt
scotswheatlippies scotswheatlippy
scotswheatpeck 4 scotswheatlippy
scotswheatfirlot 4 scotswheatpeck
scotswheatboll 4 scotswheatfirlot
scotswheatchalder 16 scotswheatboll
scotsoatlippy 200.345 UKinch^3 # Also used for barley and malt
scotsoatlippies scotsoatlippy
scotsoatpeck 4 scotsoatlippy
scotsoatfirlot 4 scotsoatpeck
scotsoatboll 4 scotsoatfirlot
scotsoatchalder 16 scotsoatboll
# Scots Tron weight
trondrop 1|16 tronounce
tronounce 1|20 tronpound
tronpound 9520 grain
tronstone 16 tronpound
# Irish liquid capacity measure
irishnoggin 1|4 irishpint
irishpint 1|2 irishquart
irishquart 1|2 irishpottle
irishpottle 1|2 irishgallon
irishgallon 217.6 UKinch^3
irishrundlet 18 irishgallon
irishbarrel 31.5 irishgallon
irishtierce 42 irishgallon
irishhogshead 2 irishbarrel
irishpuncheon 2 irishtierce
irishpipe 2 irishhogshead
irishtun 2 irishpipe
# Irish dry capacity measure
irishpeck 2 irishgallon
irishbushel 4 irishpeck
irishstrike 2 irishbushel
irishdrybarrel 2 irishstrike
irishquarter 2 irishbarrel
# English Tower weights, abolished in 1528
towerpound 5400 grain
towerounce 1|12 towerpound
towerpennyweight 1|20 towerounce
towergrain 1|32 towerpennyweight
# English Mercantile weights, used since the late 12th century
mercpound 6750 grain
mercounce 1|15 mercpound
mercpennyweight 1|20 mercounce
# English weights for lead
leadstone 12.5 lb
fotmal 70 lb
leadwey 14 leadstone
fothers 12 leadwey
# English Hay measure
newhaytruss 60 lb # New and old here seem to refer to "new"
newhayload 36 newhaytruss # hay and "old" hay rather than a new unit
oldhaytruss 56 lb # and an old unit.
oldhayload 36 oldhaytruss
# English wool measure
woolclove 7 lb
woolstone 2 woolclove
wooltod 2 woolstone
woolwey 13 woolstone
woolsack 2 woolwey
woolsarpler 2 woolsack
woollast 6 woolsarpler
#
# Ancient history units: There tends to be uncertainty in the definitions
# of the units in this section
# These units are from [11]
# Roman measure. The Romans had a well defined distance measure, but their
# measures of weight were poor. They adopted local weights in different
# regions without distinguishing among them so that there are half a dozen
# different Roman "standard" weight systems.
romanfoot 296 mm # There is some uncertainty in this definition
romanfeet romanfoot # from which all the other units are derived.
pes romanfoot # This value appears in numerous sources. In "The
pedes romanfoot # Roman Land Surveyors", Dilke gives 295.7 mm.
romaninch 1|12 romanfoot # The subdivisions of the Roman foot have the
romandigit 1|16 romanfoot # same names as the subdivisions of the pound,
romanpalm 1|4 romanfoot # but we can't have the names for different
romancubit 18 romaninch # units.
romanpace 5 romanfeet # Roman double pace (basic military unit)
passus romanpace
romanperch 10 romanfeet
stade 125 romanpaces
stadia stade
stadium stade
romanmile 8 stadia # 1000 paces
romanleague 1.5 romanmile
schoenus 4 romanmile
# Other values for the Roman foot (from Dilke)
earlyromanfoot 29.73 cm
pesdrusianus 33.3 cm # or 33.35 cm, used in Gaul & Germany in 1st c BC
lateromanfoot 29.42 cm
# Roman areas
actuslength 120 romanfeet # length of a Roman furrow
actus 120*4 romanfeet^2 # area of the furrow
squareactus 120^2 romanfeet^2 # actus quadratus
acnua squareactus
iugerum 2 squareactus
iugera iugerum
jugerum iugerum
jugera iugerum
heredium 2 iugera # heritable plot
heredia heredium
centuria 100 heredia
centurium centuria
# Roman volumes
sextarius 35.4 in^3 # Basic unit of Roman volume. As always,
sextarii sextarius # there is uncertainty. Six large Roman
# measures survive with volumes ranging from
# 34.4 in^3 to 39.55 in^3. Three of them
# cluster around the size given here.
#
# But the values for this unit vary wildly
# in other sources. One reference gives 0.547
# liters, but then says the amphora is a
# cubic Roman foot. This gives a value for the
# sextarius of 0.540 liters. And the
# encyclopedia Britannica lists 0.53 liters for
# this unit. Both [7] and [11], which were
# written by scholars of weights and measures,
# give the value of 35.4 cubic inches.
cochlearia 1|48 sextarius
cyathi 1|12 sextarius
acetabula 1|8 sextarius
quartaria 1|4 sextarius
quartarius quartaria
heminae 1|2 sextarius
hemina heminae
cheonix 1.5 sextarii
# Dry volume measures (usually)
semodius 8 sextarius
semodii semodius
modius 16 sextarius
modii modius
# Liquid volume measures (usually)
congius 12 heminae
congii congius
amphora 8 congii
amphorae amphora # Also a dry volume measure
culleus 20 amphorae
quadrantal amphora
# Roman weights
libra 5052 grain # The Roman pound varied significantly
librae libra # from 4210 grains to 5232 grains. Most of
romanpound libra # the standards were obtained from the weight
uncia 1|12 libra # of particular coins. The one given here is
unciae uncia # based on the Gold Aureus of Augustus which
romanounce uncia # was in use from BC 27 to AD 296.
deunx 11 uncia
dextans 10 uncia
dodrans 9 uncia
bes 8 uncia
seprunx 7 uncia
semis 6 uncia
quincunx 5 uncia
triens 4 uncia
quadrans 3 uncia
sextans 2 uncia
sescuncia 1.5 uncia
semuncia 1|2 uncia
siscilius 1|4 uncia
sextula 1|6 uncia
semisextula 1|12 uncia
scriptulum 1|24 uncia
scrupula scriptulum
romanobol 1|2 scrupula
romanaspound 4210 grain # Old pound based on bronze coinage, the
# earliest money of Rome BC 338 to BC 268.
# Egyptian length measure
egyptianroyalcubit 20.63 in # plus or minus .2 in
egyptianpalm 1|7 egyptianroyalcubit
egyptiandigit 1|4 egyptianpalm
egyptianshortcubit 6 egyptianpalm
doubleremen 29.16 in # Length of the diagonal of a square with
remendigit 1|40 doubleremen # side length of 1 royal egyptian cubit.
# This is divided into 40 digits which are
# not the same size as the digits based on
# the royal cubit.
# Greek length measures
greekfoot 12.45 in # Listed as being derived from the
greekfeet greekfoot # Egyptian Royal cubit in [11]. It is
greekcubit 1.5 greekfoot # said to be 3|5 of a 20.75 in cubit.
pous greekfoot
podes greekfoot
orguia 6 greekfoot
greekfathom orguia
stadion 100 orguia
akaina 10 greekfeet
plethron 10 akaina
greekfinger 1|16 greekfoot
homericcubit 20 greekfingers # Elbow to end of knuckles.
shortgreekcubit 18 greekfingers # Elbow to start of fingers.
ionicfoot 296 mm
doricfoot 326 mm
olympiccubit 25 remendigit # These olympic measures were not as
olympicfoot 2|3 olympiccubit # common as the other greek measures.
olympicfinger 1|16 olympicfoot # They were used in agriculture.
olympicfeet olympicfoot
olympicdakylos olympicfinger
olympicpalm 1|4 olympicfoot
olympicpalestra olympicpalm
olympicspithame 3|4 foot
olympicspan olympicspithame
olympicbema 2.5 olympicfeet
olympicpace olympicbema
olympicorguia 6 olympicfeet
olympicfathom olympicorguia
olympiccord 60 olympicfeet
olympicamma olympiccord
olympicplethron 100 olympicfeet
olympicstadion 600 olympicfeet
# Greek capacity measure
greekkotyle 270 ml # This approximate value is obtained
xestes 2 greekkotyle # from two earthenware vessels that
khous 12 greekkotyle # were reconstructed from fragments.
metretes 12 khous # The kotyle is a day's corn ration
choinix 4 greekkotyle # for one man.
hekteos 8 choinix
medimnos 6 hekteos
# Greek weight. Two weight standards were used, an Aegina standard based
# on the Beqa shekel and an Athens (attic) standard.
aeginastater 192 grain # Varies up to 199 grain
aeginadrachmae 1|2 aeginastater
aeginaobol 1|6 aeginadrachmae
aeginamina 50 aeginastaters
aeginatalent 60 aeginamina # Supposedly the mass of a cubic foot
# of water (whichever foot was in use)
atticstater 135 grain # Varies 134-138 grain
atticdrachmae 1|2 atticstater
atticobol 1|6 atticdrachmae
atticmina 50 atticstaters
attictalent 60 atticmina # Supposedly the mass of a cubic foot
# of water (whichever foot was in use)
# "Northern" cubit and foot. This was used by the pre-Aryan civilization in
# the Indus valley. It was used in Mesopotamia, Egypt, North Africa, China,
# central and Western Europe until modern times when it was displaced by
# the metric system.
northerncubit 26.6 in # plus/minus .2 in
northernfoot 1|2 northerncubit
sumeriancubit 495 mm
kus sumeriancubit
sumerianfoot 2|3 sumeriancubit
assyriancubit 21.6 in
assyrianfoot 1|2 assyriancubit
assyrianpalm 1|3 assyrianfoot
assyriansusi 1|20 assyrianpalm
susi assyriansusi
persianroyalcubit 7 assyrianpalm
# Arabic measures. The arabic standards were meticulously kept. Glass weights
# accurate to .2 grains were made during AD 714-900.
hashimicubit 25.56 in # Standard of linear measure used
# in Persian dominions of the Arabic
# empire 7-8th cent. Is equal to two
# French feet.
blackcubit 21.28 in
arabicfeet 1|2 blackcubit
arabicfoot arabicfeet
arabicinch 1|12 arabicfoot
arabicmile 4000 blackcubit
silverdirhem 45 grain # The weights were derived from these two
tradedirhem 48 grain # units with two identically named systems
# used for silver and used for trade purposes
silverkirat 1|16 silverdirhem
silverwukiyeh 10 silverdirhem
silverrotl 12 silverwukiyeh
arabicsilverpound silverrotl
tradekirat 1|16 tradedirhem
tradewukiyeh 10 tradedirhem
traderotl 12 tradewukiyeh
arabictradepound traderotl
# Miscellaneous ancient units
parasang 3.5 mile # Persian unit of length usually thought
# to be between 3 and 3.5 miles
biblicalcubit 21.8 in
hebrewcubit 17.58 in
li 10|27.8 mile # Chinese unit of length
# 100 li is considered a day's march
liang 11|3 oz # Chinese weight unit
# Medieval time units. According to the OED, these appear in Du Cange
# by Papias.
timepoint 1|5 hour # also given as 1|4
timeminute 1|10 hour
timeostent 1|60 hour
timeounce 1|8 timeostent
timeatom 1|47 timeounce
# Given in [15], these subdivisions of the grain were supposedly used
# by jewelers. The mite may have been used but the blanc could not
# have been accurately measured.
mite 1|20 grain
droit 1|24 mite
periot 1|20 droit
blanc 1|24 periot
#
# Localization
#
!var UNITS_ENGLISH US
hundredweight ushundredweight
ton uston
scruple apscruple
fluidounce usfluidounce
gallon usgallon
bushel usbushel
quarter quarterweight
cup uscup
tablespoon ustablespoon
teaspoon usteaspoon
dollar US$
cent $ 0.01
penny cent
minim minimvolume
pony ponyvolume
grand usgrand
firkin usfirkin
hogshead ushogshead
cable uscable
!endvar
!var UNITS_ENGLISH GB
hundredweight brhundredweight
ton brton
scruple brscruple
fluidounce brfluidounce
gallon brgallon
bushel brbushel
quarter brquarter
chaldron brchaldron
cup brcup
teacup brteacup
tablespoon brtablespoon
teaspoon brteaspoon
dollar US$
cent $ 0.01
penny brpenny
minim minimnote
pony brpony
grand brgrand
firkin brfirkin
hogshead brhogshead
cable brcable
!endvar
!varnot UNITS_ENGLISH GB US
!message Unknown value for environment variable UNITS_ENGLISH. Should be GB or US.
!endvar
!utf8
⅛- 1|8
¼- 1|4
⅜- 3|8
½- 1|2
⅝- 5|8
¾- 3|4
⅞- 7|8
⅙- 1|6
⅓- 1|3
⅔- 2|3
⅚- 5|6
⅕- 1|5
⅖- 2|5
⅗- 3|5
⅘- 4|5
# U+2150- 1|7 For some reason these characters are getting
# U+2151- 1|9 flagged as invalid UTF8.
# U+2152- 1|10
#⅐- 1|7 # fails under MacOS
#⅑- 1|9 # fails under MacOS
#⅒- 1|10 # fails under MacOS
ℯ exp(1) # U+212F, base of natural log
µ- micro # micro sign U+00B5
μ- micro # small mu U+03BC
ångström angstrom
Å angstrom # angstrom symbol U+212B
Å angstrom # A with ring U+00C5
röntgen roentgen
K K # Kelvin symbol, U+212A
℃ degC
℉ degF
°C degC
°F degF
°K K # °K is incorrect notation
°R degR
ℓ liter # unofficial abbreviation used in some places
Ω ohm # Ohm symbol U+2126
Ω ohm # Greek capital omega U+03A9
℧ mho
G₀ G0
H₀ H0
Z₀ Z0
a₀ a0
n₀ n0
ε₀ epsilon0
μ₀ mu0
Φ₀ Phi0
R∞ Rinfinity
R_∞ Rinfinity
λ_C lambda_C
μ_B mu_B
ν_133Cs nu_133Cs
ʒ dram # U+0292
℈ scruple
℥ ounce
℔ lb
ℎ h
ℏ hbar
τ tau
π pi # Greek letter pi
𝜋 pi # mathematical italic small pi
α alpha
σ sigma
‰ 1|1000
‱ 1|10000
#
# Unicode currency symbols
#
¢ cent
£ britainpound
¥ japanyen
€ euro
₩ southkoreawon
₪ israelnewshekel
₤ lira
# ₺ turkeylira # fails under MacOS
₨ rupee # unofficial legacy rupee sign
# ₹ indiarupee # official rupee sign # MacOS fail
#؋ afghanafghani # fails under MacOS
฿ thailandbaht
₡ costaricacolon
₣ francefranc
₦ nigerianaira
₧ spainpeseta
₫ vietnamdong
₭ laokip
₮ mongoliatugrik
₯ greecedrachma
₱ philippinepeso
# ₲ paraguayguarani # fails under MacOS
#₴ ukrainehryvnia # fails under MacOS
#₵ ghanacedi # fails under MacOS
#₸ kazakhstantenge # fails under MacOS
#₼ azerbaijanmanat # fails under MacOS
#₽ russiaruble # fails under MacOS
#₾ georgialari # fails under MacOS
﷼ iranrial
﹩ $
¢ ¢
£ £
¥ ¥
₩ ₩
#
# Square Unicode symbols starting at U+3371
#
㍱ hPa
㍲ da
㍳ au
㍴ bar
# ㍵ oV???
㍶ pc
#㍷ dm invalid on Mac
#㍸ dm^2 invalid on Mac
#㍹ dm^3 invalid on Mac
㎀ pA
㎁ nA
㎂ µA
㎃ mA
㎄ kA
㎅ kB
㎆ MB
㎇ GB
㎈ cal
㎉ kcal
㎊ pF
㎋ nF
㎌ µF
㎍ µg
㎎ mg
㎏ kg
㎐ Hz
㎑ kHz
㎒ MHz
㎓ GHz
㎔ THz
㎕ µL
㎖ mL
㎗ dL
㎘ kL
㎙ fm
㎚ nm
㎛ µm
㎜ mm
㎝ cm
㎞ km
㎟ mm^2
㎠ cm^2
㎡ m^2
㎢ km^2
㎣ mm^3
㎤ cm^3
㎥ m^3
㎦ km^3
㎧ m/s
㎨ m/s^2
㎩ Pa
㎪ kPa
㎫ MPa
㎬ GPa
㎭ rad
㎮ rad/s
㎯ rad/s^2
㎰ ps
㎱ ns
㎲ µs
㎳ ms
㎴ pV
㎵ nV
㎶ µV
㎷ mV
㎸ kV
㎹ MV
㎺ pW
㎻ nW
㎼ µW
㎽ mW
㎾ kW
㎿ MW
㏀ kΩ
㏁ MΩ
㏃ Bq
㏄ cc
㏅ cd
㏆ C/kg
㏈() dB
㏉ Gy
㏊ ha
# ㏋ HP??
㏌ in
# ㏍ KK??
# ㏎ KM???
㏏ kt
㏐ lm
# ㏑ ln
# ㏒ log
㏓ lx
㏔ mb
㏕ mil
㏖ mol
㏗() pH
㏙ ppm
# ㏚ PR???
㏛ sr
㏜ Sv
㏝ Wb
#㏞ V/m Invalid on Mac
#㏟ A/m Invalid on Mac
#㏿ gal Invalid on Mac
!endutf8
############################################################################
#
# Unit list aliases
#
# These provide a shorthand for conversions to unit lists.
#
############################################################################
!unitlist uswt lb;oz
!unitlist hms hr;min;sec
!unitlist time year;day;hr;min;sec
!unitlist dms deg;arcmin;arcsec
!unitlist ftin ft;in;1|8 in
!unitlist ftin4 ft;in;1|4 in
!unitlist ftin8 ft;in;1|8 in
!unitlist ftin16 ft;in;1|16 in
!unitlist ftin32 ft;in;1|32 in
!unitlist ftin64 ft;in;1|64 in
!unitlist inchfine in;1|8 in;1|16 in;1|32 in;1|64 in
!unitlist by2 1;1|2;1|4;1|8;1|16;1|32;1|64;1|128;1|256
!unitlist usvol cup;3|4 cup;2|3 cup;1|2 cup;1|3 cup;1|4 cup;\
tbsp;tsp;1|2 tsp;1|4 tsp;1|8 tsp
############################################################################
#
# The following units were in the Unix units database but do not appear in
# this file:
#
# wey used for cheese, salt and other goods. Measured mass or
# waymass volume depending on what was measured and where the measuring
# took place. A wey of cheese ranged from 200 to 324 pounds.
#
# sack No precise definition
#
# spindle The length depends on the type of yarn
#
# block Defined variously on different computer systems
#
# erlang A unit of telephone traffic defined variously.
# Omitted because there are no other units for this
# dimension. Is this true? What about CCS = 1/36 erlang?
# Erlang is supposed to be dimensionless. One erlang means
# a single channel occupied for one hour.
#
############################################################################
#
# The following have been suggested or considered and deemed out of scope.
# They will not be added to GNU units.
#
# Conversions between different calendar systems used in different countries or
# different historical periods are out of scope for units and will not be added.
#
# Wind chill and heat index cannot be handled because they are bivarite,
# with dependence on both the temperature and wind speed or humidity.
#
# Plain english text output like "one hectare is equivalent to one hundred
# million square centimeters" is out of scope.
#
|