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
|
*=======================================================================
*
* PGSBOX 4.8 - draw curvilinear coordinate axes for PGPLOT.
* Copyright (C) 1997-2011, Mark Calabretta
*
* This file is part of PGSBOX.
*
* PGSBOX is free software: you can redistribute it and/or modify it
* under the terms of the GNU Lesser General Public License as published
* by the Free Software Foundation, either version 3 of the License, or
* (at your option) any later version.
*
* PGSBOX 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 Lesser General Public
* License for more details.
*
* You should have received a copy of the GNU Lesser General Public
* License along with PGSBOX. If not, see http://www.gnu.org/licenses.
*
* Correspondence concerning PGSBOX may be directed to:
* Internet email: mcalabre@atnf.csiro.au
* Postal address: Dr. Mark Calabretta
* Australia Telescope National Facility, CSIRO
* PO Box 76
* Epping NSW 1710
* AUSTRALIA
*
* Author: Mark Calabretta, Australia Telescope National Facility
* http://www.atnf.csiro.au/~mcalabre/index.html
* $Id: pgcrfn.f,v 4.8.1.1 2011/08/15 08:07:07 cal103 Exp cal103 $
*=======================================================================
*
* PGCRFN defines separable pairs of non-linear coordinate systems for
* PGSBOX.
*
* Given:
* OPCODE I Transformation code:
* +2: Compute a set of pixel coordinates that
* describe a path between this and the
* previous pair of world coordinates
* remembered from the last call with
* OPCODE = +1 or +2.
* +1: Compute pixel coordinates from world
* coordinates.
* 0: Initialize.
* -1: Compute world coordinates from pixel
* coordinates.
*
* NLC I Number of elements in FCODE (=8).
*
* NLI I Number of elements in NLIPRM (=2).
*
* NLD I Number of elements in NLDPRM.
*
* FCODE C(NLC)*1 Character array (contains the CTYPE array,
* see below).
*
* Given and/or returned:
* NLIPRM I(NLI) Integer coefficients (see below).
*
* NLDPRM D(2,NLD) Double precision coefficients (see below).
*
* WORLD D(2) World coordinates.
* Given if OPCODE > 0, returned if OPCODE < 0.
*
* PIXEL D(2) Pixel coordinates.
* Given if OPCODE < 0, returned if OPCODE > 0.
*
* CONTRL I Control flag for OPCODE = +2 (ignored, always
* set to 0 on return).
*
* CONTXT D(20) Context elements (ignored).
*
* Returned:
* IERR I Status return value:
* 0: Success.
* 1: Invalid parameters.
* 2: Invalid world coordinate.
* 3: Invalid pixel coordinate.
*
* Notes:
* PGCRFN assumes a simple 2-D image. The FCODE array contains
* two four-character mnemonics that select function types:
*
* "Lin " Linear
* "Log " Logarithmic
* "Pow " Power law
*
* The first two elements of NLIPRM are set on initialization to
* offsets used by computed GO TOs for each function type.
*
* Note that PGCRFN treats NLDPRM as an array of dimension two.
* The NLDPRM are used as follows:
*
* Type WORLD(J) =
* Lin NLDPRM(J,3) + S
* Log NLDPRM(J,3) * LOG10(S)
* Pow (NLDPRM(J,3) + S)**NLDPRM(J,4)
*
* Where in each case S = NLDPRM(J,2)*(PIXEL(J) - NLDPRM(J,1))
*
*=======================================================================
SUBROUTINE PGCRFN (OPCODE, NLC, NLI, NLD, FCODE, NLIPRM, NLDPRM,
: WORLD, PIXEL, CONTRL, CONTXT, IERR)
*-----------------------------------------------------------------------
INTEGER CONTRL, IERR, J, NLC, NLD, NLI, OPCODE, NLIPRM(NLI)
DOUBLE PRECISION CONTXT(20), NLDPRM(2,NLD), PIXEL(2), S, WORLD(2)
CHARACTER FCODE(2)*4, FCODES*20
DATA FCODES(1:20) /'Lin Log Pow '/
*-----------------------------------------------------------------------
IERR = 0
IF (OPCODE.GT.0) THEN
* Compute pixel coordinates from world coordinates.
DO 200 J = 1, 2
GO TO (110, 120, 130) NLIPRM(J)
IERR = 1
RETURN
* Linear.
110 S = WORLD(J) - NLDPRM(J,3)
GO TO 190
* Logarithmic to base 10.
120 S = 10D0**(WORLD(J)/NLDPRM(J,3))
GO TO 190
* Power.
130 S = WORLD(J)**(1D0/NLDPRM(J,4)) - NLDPRM(J,3)
190 PIXEL(J) = NLDPRM(J,1) + S/NLDPRM(J,2)
200 CONTINUE
CONTRL = 0
ELSE IF (OPCODE.EQ.0) THEN
* Initialize.
IF (NLC.LT.8 .OR. NLI.LT.2 .OR. NLD.LT.3) THEN
IERR = 1
RETURN
END IF
* Compute pointers.
NLIPRM(1) = (INDEX(FCODES,FCODE(1)) + 3)/4
NLIPRM(2) = (INDEX(FCODES,FCODE(2)) + 3)/4
IF (NLIPRM(1).EQ.0 .OR. NLIPRM(2).EQ.0) THEN
IERR = 1
RETURN
END IF
CONTRL = 0
ELSE IF (OPCODE.EQ.-1) THEN
* Compute world coordinates from pixel coordinates.
DO 300 J = 1, 2
S = NLDPRM(J,2)*(PIXEL(J) - NLDPRM(J,1))
GO TO (210, 220, 230) NLIPRM(J)
IERR = 1
RETURN
* Linear.
210 WORLD(J) = NLDPRM(J,3) + S
GO TO 300
* Logarithmic to base 10.
220 IF (S.LE.0D0) THEN
IERR = 1
RETURN
END IF
WORLD(J) = NLDPRM(J,3)*LOG10(S)
GO TO 300
* Power.
230 S = S + NLDPRM(J,3)
IF (S.LE.0D0 .AND. MOD(NLDPRM(J,4),1D0).NE.0D0) THEN
IERR = 1
RETURN
END IF
WORLD(J) = S**NLDPRM(J,4)
300 CONTINUE
ELSE
IERR = 1
END IF
RETURN
END
|