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# $Id: xw29.py 11680 2011-03-27 17:57:51Z airwin $
# Copyright (C) 2008 Andrew Ross
# Sample plots using date / time formatting for axes
#
# This file is part of PLplot.
#
# PLplot is free software; you can redistribute it and/or modify
# it under the terms of the GNU Library General Public License as published
# by the Free Software Foundation; either version 2 of the License, or
# (at your option) any later version.
#
# PLplot 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 Library General Public License for more details.
#
# You should have received a copy of the GNU Library General Public License
# along with PLplot; if not, write to the Free Software
# Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301 USA
#
from plplot_py_demos import *
import calendar
#--------------------------------------------------------------------------
# main
#
# Draws several plots which demonstrate the use of date / time formats for
# the axis labels.
# Time formatting is done using the system strftime routine. See the
# documentation of this for full details of the available formats.
#
# 1) Plotting temperature over a day (using hours / minutes)
# 2) Plotting
#
# Note: Times are stored as seconds since the epoch (usually 1st Jan 1970).
#
#--------------------------------------------------------------------------
def main():
plsesc('@')
plot1()
plot2()
plot3()
plot4()
# Plot a model diurnal cycle of temperature
def plot1():
# Data points every 10 minutes for 1 day
npts = 73;
xmin = 0.0;
xmax = 60.0*60.0*24.0; # Number of seconds in a day
ymin = 10.0;
ymax = 20.0;
x = xmax*arange(npts)/float(npts)
y = 15.0 - 5.0*cos(2*pi*x/xmax)
xerr1 = x-60.0*5.0
xerr2 = x+60.0*5.0
yerr1 = y-0.1
yerr2 = y+0.1
pladv(0)
plsmaj(0.0,0.5)
plsmin(0.0,0.5)
plvsta()
plwind(xmin, xmax, ymin, ymax)
# Draw a box with ticks spaced every 3 hour in X and 1 degree C in Y.
plcol0(1)
# Set time format to be hours:minutes
pltimefmt("%H:%M")
plbox("bcnstd", 3.0*60*60, 3, "bcnstv", 1, 5)
plcol0(3)
pllab("Time (hours:mins)", "Temperature (degC)", "@frPLplot Example 29 - Daily temperature")
plcol0(4)
plline(x, y)
plcol0(2)
plerrx(xerr1,xerr2,y)
plcol0(3)
plerry(x,yerr1,yerr2)
plsmin(0.0,1.0)
plsmaj(0.0,1.0)
# Plot the number of hours of daylight as a function of day for a year
def plot2():
# Latitude for London
lat = 51.5
npts = 365
xmin = 0.0
xmax = npts*60.0*60.0*24.0
ymin = 0.0
ymax = 24.0
# Formula for hours of daylight from
# "A Model Comparison for Daylength as a Function of Latitude and
# Day of the Year", 1995, Ecological Modelling, 80, pp 87-95.
x = arange(npts)*60.0*60.0*24.0
p = arcsin(0.39795*cos(0.2163108 + 2*arctan(0.9671396*tan(0.00860*(arange(npts)-186)))))
d = 24.0 - (24.0/pi)*arccos( (sin(0.8333*pi/180.0) + sin(lat*pi/180.0)*sin(p)) / (cos(lat*pi/180.0)*cos(p)) )
y = d
plcol0(1)
# Set time format to be abbreviated month name followed by day of month
pltimefmt("%b %d")
plprec(1,1)
plenv(xmin, xmax, ymin, ymax, 0, 40)
plcol0(3)
pllab("Date", "Hours of daylight", "@frPLplot Example 29 - Hours of daylight at 51.5N")
plcol0(4)
plline(x, y)
plprec(0,0)
def plot3():
# number of seconds elapsed since the Unix epoch (1970-01-01, UTC) for
# 2005-12-01, UTC.
xmin = plctime(2005,11,1,0,0,0.)
npts = 62
xmax = xmin + npts*60.0*60.0*24.0
ymin = 0.0
ymax = 5.0
i = arange(npts)
imin = float(npts)/2.0-abs(i - float(npts)/2.0)
x = xmin + i*60.0*60.0*24.0
y = 1.0 + sin(2*pi*i/7.0) + exp( imin / 31.0)
pladv(0)
plvsta()
plwind(xmin, xmax, ymin, ymax)
plcol0(1)
# Set time format to be ISO 8601 standard YYYY-MM-DD. Note that this is
# equivalent to %f for C99 compliant implementations of strftime.
pltimefmt("%Y-%m-%d")
# Draw a box with ticks spaced every 14 days in X and 1 hour in Y.
plbox("bcnstd", 14*24.0*60.0*60.0,14, "bcnstv", 1, 4)
plcol0(3)
pllab("Date", "Hours of television watched", "@frPLplot Example 29 - Hours of television watched in Dec 2005 / Jan 2006")
plcol0(4)
plssym(0.0,0.5)
plpoin(x, y, 2)
plline(x, y)
def plot4():
# TAI-UTC (seconds) as a function of time.
# Use Besselian epochs as the continuous time interval just to prove
# this does not introduce any issues.
# Use the definition given in http://en.wikipedia.org/wiki/Besselian_epoch
#
# B = 1900. + (JD -2415020.31352)/365.242198781
# ==> (as calculated with aid of "bc -l" command)
# B = (MJD + 678940.364163900)/365.242198781
# ==>
# MJD = B*365.24219878 - 678940.364163900
scale = 365.242198781
offset1 = -678940.
offset2 = -0.3641639
plconfigtime(scale, offset1, offset2, 0x0, 0, 0, 0, 0, 0, 0, 0.)
for kind in range(7):
if kind == 0:
xmin = plctime(1950,0,2,0,0,0.)
xmax = plctime(2020,0,2,0,0,0.)
npts = 70*12 + 1
ymin = 0.0
ymax = 36.0
time_format = "%Y%"
if_TAI_time_format = True
title_suffix = "from 1950 to 2020"
xtitle = "Year"
xlabel_step = 10.
elif kind == 1 or kind ==2:
xmin = plctime(1961,7,1,0,0,1.64757-.20)
xmax = plctime(1961,7,1,0,0,1.64757+.20)
npts = 1001
ymin = 1.625
ymax = 1.725
time_format = "%S%2%"
title_suffix = "near 1961-08-01 (TAI)"
xlabel_step = 0.05/(scale*86400.)
if kind == 1:
if_TAI_time_format = True
xtitle = "Seconds (TAI)"
else:
if_TAI_time_format = False
xtitle = "Seconds (TAI) labelled with corresponding UTC"
elif kind == 3 or kind ==4:
xmin = plctime(1963,10,1,0,0,2.6972788-.20)
xmax = plctime(1963,10,1,0,0,2.6972788+.20)
npts = 1001
ymin = 2.55
ymax = 2.75
time_format = "%S%2%"
title_suffix = "near 1963-11-01 (TAI)"
xlabel_step = 0.05/(scale*86400.)
if kind == 3:
if_TAI_time_format = True
xtitle = "Seconds (TAI)"
else:
if_TAI_time_format = False
xtitle = "Seconds (TAI) labelled with corresponding UTC"
elif kind == 5 or kind == 6:
xmin = plctime(2009,0,1,0,0,34.-5.)
xmax = plctime(2009,0,1,0,0,34.+5.)
npts = 1001
ymin = 32.5
ymax = 34.5
time_format = "%S%2%"
title_suffix = "near 2009-01-01 (TAI)"
xlabel_step = 1./(scale*86400.)
if kind == 5:
if_TAI_time_format = True
xtitle = "Seconds (TAI)"
else:
if_TAI_time_format = False
xtitle = "Seconds (TAI) labelled with corresponding UTC"
i = arange(npts)
x = xmin + i*(xmax-xmin)/float(npts-1)
y = zeros(npts)
for j in range(npts):
plconfigtime(scale, offset1, offset2, 0x0, 0, 0, 0, 0, 0, 0, 0.)
tai = x[j]
(tai_year, tai_month, tai_day, tai_hour, tai_min, tai_sec) = plbtime(tai)
plconfigtime(scale, offset1, offset2, 0x2, 0, 0, 0, 0, 0, 0, 0.)
(utc_year, utc_month, utc_day, utc_hour, utc_min, utc_sec) = plbtime(tai)
plconfigtime(scale, offset1, offset2, 0x0, 0, 0, 0, 0, 0, 0, 0.)
utc = plctime(utc_year, utc_month, utc_day, utc_hour, utc_min, utc_sec)
y[j]=(tai-utc)*scale*86400.
pladv(0)
plvsta()
plwind(xmin, xmax, ymin, ymax)
plcol0(1)
if if_TAI_time_format:
plconfigtime(scale, offset1, offset2, 0x0, 0, 0, 0, 0, 0, 0, 0.)
else:
plconfigtime(scale, offset1, offset2, 0x2, 0, 0, 0, 0, 0, 0, 0.)
pltimefmt(time_format)
plbox("bcnstd", xlabel_step, 0, "bcnstv", 0., 0)
plcol0(3)
pllab(xtitle, "TAI-UTC (sec)", "@frPLplot Example 29 - TAI-UTC " + title_suffix)
plcol0(4)
plline(x, y)
main()
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