This file is indexed.

/usr/share/doc/libplplot12/examples/f95/x29f.f90 is in libplplot-dev 5.10.0+dfsg2-0.1ubuntu2.

This file is owned by root:root, with mode 0o644.

The actual contents of the file can be viewed below.

  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
!  $Id: x29f.f90 11977 2011-10-19 14:43:26Z andrewross $
!
!   Sample plots using date / time formatting for axes
!
!   Copyright (C) 2008  Andrew Ross
!
!   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
!

   program x29f95
   use plplot

   implicit none

   real(kind=plflt), dimension(365) :: x, y, xerr1, xerr2, yerr1, yerr2
   common /plotdat/ x, y, xerr1, xerr2, yerr1, yerr2

   call plparseopts(PL_PARSE_FULL)
   
   call plinit()

!  This is the ASCII value for character @
   call plsesc(64)
   
   call plot1()
   call plot2()
   call plot3()
   call plot4()
   
   call plend()
   end program x29f95

!====================================================================
!
!     Plot a model diurnal cycle of temperature
     
      subroutine plot1()
      use plplot, PI => PL_PI
      implicit none

      real(kind=plflt), dimension(365) :: x, y, xerr1, xerr2, yerr1, yerr2
      common /plotdat/ x, y, xerr1, xerr2, yerr1, yerr2

      integer :: i, npts
      real(kind=plflt) :: xmin, xmax, ymin, ymax
      
      parameter(npts = 73)
      parameter(xmin = 0.0_plflt)
      parameter(xmax = 60.0_plflt*60.0_plflt*24.0_plflt)
      parameter(ymin = 10.0_plflt)
      parameter(ymax = 20.0_plflt)

      do i = 1,npts
         x(i) = xmax*(dble(i-1)/dble(npts))
         y(i) = 15.0_plflt - 5.0_plflt*cos(2.0_plflt*PI*dble(i-1)/dble(npts))
!     Set x error bars to +/- 5 minute 
         xerr1(i) = x(i)-60.0_plflt*5.0_plflt
         xerr2(i) = x(i)+60.0_plflt*5.0_plflt
!     Set y error bars to +/- 0.1 deg C
         yerr1(i) = y(i)-0.1_plflt
         yerr2(i) = y(i)+0.1_plflt
      enddo

      call pladv(0)
      
!     Rescale major ticks marks by 0.5
      call plsmaj(0.0_plflt,0.5_plflt)
!     Rescale minor ticks and error bar marks by 0.5
      call plsmin(0.0_plflt,0.5_plflt)

      call plvsta()
      call plwind(xmin, xmax, ymin, ymax)

!     Draw a box with ticks spaced every 3 hour in X and 1 degree C in Y.
      call plcol0(1)
!     Set time format to be hours:minutes
      call pltimefmt("%H:%M")
      call plbox("bcnstd", 3.0_plflt*60.0_plflt*60.0_plflt, 3, "bcnstv", &
           1.0_plflt, 5)

      call plcol0(3)
      call pllab("Time (hours:mins)", "Temperature (degC)", &
           "@frPLplot Example 29 - Daily temperature")
      
      call plcol0(4)

      call plline(x(1:npts), y(1:npts))
      call plcol0(2)
      call plerrx(xerr1(1:npts), xerr2(1:npts), y(1:npts))
      call plcol0(3)
      call plerry(x(1:npts), yerr1(1:npts), yerr2(1:npts))

!     Rescale major / minor tick marks back to default
      call plsmin(0.0_plflt,1.0_plflt)
      call plsmaj(0.0_plflt,1.0_plflt)
      
    end subroutine plot1

!
!     Plot the number of hours of daylight as a function of day for a year
!
      subroutine plot2() 
      use plplot, PI => PL_PI

      implicit none
      
      integer ::  j, npts
      real(kind=plflt) :: xmin, xmax, ymin, ymax
      real(kind=plflt) :: lat, p, d
      real(kind=plflt), dimension(365) :: x, y, xerr1, xerr2, yerr1, yerr2
      common /plotdat/ x, y, xerr1, xerr2, yerr1, yerr2


      ! Latitude for London
      parameter (lat = 51.5_plflt)
      
      parameter (npts = 365)
      
      parameter(xmin = 0.0_plflt)
      parameter(xmax = npts*60.0_plflt*60.0_plflt*24.0_plflt)
      parameter(ymin = 0)
      parameter(ymax = 24)

!     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.
      do j=1,npts
         x(j) = (j-1)*60.0_plflt*60.0_plflt*24.0_plflt
         p = asin(0.39795_plflt*cos(0.2163108_plflt + 2.0_plflt* &
              atan(0.9671396_plflt*tan(0.00860_plflt*(j-187)))))
         d = 24.0_plflt - (24.0_plflt/PI)* &
              acos( (sin(0.8333_plflt*PI/180.0_plflt) + &
              sin(lat*PI/180.0_plflt)*sin(p)) / (cos(lat*PI/180.0_plflt)* &
              cos(p)) )
         y(j) = d
      enddo

      call plcol0(1)
!     Set time format to be abbreviated month name followed by day of month
      call pltimefmt("%b %d")
      call plprec(1,1)
      call plenv(xmin, xmax, ymin, ymax, 0, 40)
      
      call plcol0(3)
      call pllab("Date", "Hours of daylight", &
           "@frPLplot Example 29 - Hours of daylight at 51.5N")
  
      call plcol0(4)

      call plline(x, y)
  
      call plprec(0,0)

    end subroutine plot2

!
!
!
      subroutine plot3()
      use plplot, PI => PL_PI
      implicit none
      
      integer :: i, npts
      real(kind=plflt) :: xmin, xmax, ymin, ymax
      integer :: tstart
!      real(kind=plflt) :: toff
      real(kind=plflt), dimension(365) :: x, y, xerr1, xerr2, yerr1, yerr2
      common /plotdat/ x, y, xerr1, xerr2, yerr1, yerr2

!     integer tm(9)

      parameter (npts = 62)

!     number of seconds elapsed since the Unix epoch (1970-01-01, UTC) for
!     2005-12-01, UTC.  This is the same result as the Python
!     calendar.timegm((2005,12,1,0,0,0)) result or the Linux C timegm
!     result corresponding to 2005-12-01.
      tstart = 1133395200

      xmin = dble(tstart)
      xmax = xmin + npts*60.0_plflt*60.0_plflt*24.0_plflt
      ymin = 0.0_plflt
      ymax = 5.0_plflt
  
      do i=1,npts
         x(i) = xmin + dble(i-1)*60.0_plflt*60.0_plflt*24.0_plflt
         y(i) = 1.0_plflt + sin( 2.0_plflt*PI*dble(i-1)/7.0_plflt) + &
              exp( dble(min(i-1,npts+1-i)) / 31.0_plflt)
      enddo
      call pladv(0)

      call plvsta()
      call plwind(xmin, xmax, ymin, ymax)

      call 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.
      call pltimefmt("%Y-%m-%d")
!     Draw a box with ticks spaced every 14 days in X and 1 hour in Y.
      call plbox("bcnstd", 14.0_plflt*24.0_plflt*60.0_plflt*60.0_plflt,14, &
           "bcnstv", 1.0_plflt, 4)

      call plcol0(3)
      call pllab("Date", "Hours of television watched", &
           "@frPLplot Example 29 - Hours of television watched in " // &
           "Dec 2005 / Jan 2006")
  
      call plcol0(4)

      call plssym(0.0_plflt, 0.5_plflt)
      call plpoin(x(1:npts), y(1:npts), 2)
      call plline(x(1:npts), y(1:npts))
 
    end subroutine plot3

!
!
!
      subroutine plot4() 
      use plplot, PI => PL_PI
      implicit none

!     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.
  
      real(kind=plflt) :: scale, offset1, offset2
      real(kind=plflt) :: xmin, xmax, ymin, ymax, xlabel_step
      integer :: k, npts = 0, i
      logical :: if_TAI_time_format = .false.
      character(len=10) :: time_format
      character(len=100) :: title_suffix
      character(len=100) :: xtitle
      character(len=100) :: title
      real(kind=plflt) :: x(1001), y(1001)
      integer :: tai_year, tai_month, tai_day, tai_hour, tai_min
      real(kind=plflt) :: tai_sec, tai
      integer :: utc_year, utc_month, utc_day, utc_hour, utc_min
      real(kind=plflt) :: utc_sec, utc
      
!     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_plflt
      offset1 = -678940.0_plflt
      offset2 = -0.3641639_plflt
      call plconfigtime(scale, offset1, offset2, 0, 0, 0, 0, 0, 0, &
           0, 0._plflt)

      do k = 0,6
         if (k .eq. 0) then
            call plctime(1950,0,2,0,0,0.,xmin)
            call plctime(2020,0,2,0,0,0.,xmax)
            npts = 70*12 + 1
            ymin = 0.0_plflt
            ymax = 36.0_plflt
            time_format="%Y%"
            if_TAI_time_format = .true.
            title_suffix = "from 1950 to 2020"
            xtitle =  "Year"
            xlabel_step = 10.0_plflt
         elseif ((k .eq. 1) .or. (k .eq. 2)) then
            call plctime(1961,7,1,0,0,1.64757_plflt-.20_plflt, xmin)
            call plctime(1961,7,1,0,0,1.64757_plflt+.20_plflt, xmax)
            npts = 1001
            ymin = 1.625_plflt
            ymax = 1.725_plflt
            time_format = "%S%2%"
            title_suffix = "near 1961-08-01 (TAI)"
            xlabel_step = 0.05_plflt/(scale*86400.0_plflt)
            if (k .eq. 1) then
               if_TAI_time_format = .true.
               xtitle = "Seconds (TAI)"
            else
               if_TAI_time_format = .false.
               xtitle = "Seconds (TAI) labelled with corresponding UTC"
            endif
         elseif ((k .eq. 3) .or. (k .eq. 4)) then
            call plctime(1963,10,1,0,0,2.6972788_plflt-.20_plflt, xmin)
            call plctime(1963,10,1,0,0,2.6972788_plflt+.20_plflt, xmax)
            npts = 1001
            ymin = 2.55_plflt
            ymax = 2.75_plflt
            time_format = "%S%2%"
            title_suffix = "near 1963-11-01 (TAI)"
            xlabel_step = 0.05_plflt/(scale*86400.0_plflt)
            if (k .eq. 3) then
               if_TAI_time_format = .true.
               xtitle = "Seconds (TAI)"
            else
               if_TAI_time_format = .false.
               xtitle = "Seconds (TAI) labelled with corresponding UTC"
            endif
         elseif ((k .eq. 5) .or. (k .eq. 6)) then
            call plctime(2009,0,1,0,0,34._plflt-5._plflt,xmin)
            call plctime(2009,0,1,0,0,34._plflt+5._plflt,xmax)
            npts = 1001
            ymin = 32.5_plflt
            ymax = 34.5_plflt
            time_format = "%S%2%"
            title_suffix = "near 2009-01-01 (TAI)"
            xlabel_step = 1._plflt/(scale*86400._plflt)
            if (k .eq. 5) then
               if_TAI_time_format = .true.
               xtitle = "Seconds (TAI)"
            else 
               if_TAI_time_format = .false.
               xtitle = "Seconds (TAI) labelled with corresponding UTC"
            endif
         endif

         do i=0,npts-1
            x(i+1) = xmin + i*(xmax-xmin)/(dble(npts-1))
            call plconfigtime(scale, offset1, offset2, 0, 0, 0, 0, 0, &
                 0, 0, 0._plflt)
            tai = x(i+1)
            call plbtime(tai_year, tai_month, tai_day, tai_hour, &
                 tai_min, tai_sec, tai)
            call plconfigtime(scale, offset1, offset2, 2, 0, 0, 0, &
                 0, 0, 0, 0._plflt)
            call plbtime(utc_year, utc_month, utc_day, utc_hour, &
                 utc_min, utc_sec, tai)
            call plconfigtime(scale, offset1, offset2, 0, 0, 0, 0, &
                 0, 0, 0, 0._plflt)
            call plctime(utc_year, utc_month, utc_day, utc_hour, &
                 utc_min, utc_sec, utc)
            y(i+1)=(tai-utc)*scale*86400._plflt
         enddo

         call pladv(0)
         call plvsta()
         call plwind(xmin, xmax, ymin, ymax)
         call plcol0(1)
         if (if_TAI_time_format) then
            call plconfigtime(scale, offset1, offset2, 0, 0, 0, 0, &
                 0, 0, 0, 0._plflt)
         else
            call plconfigtime(scale, offset1, offset2, 2, 0, 0, 0, &
                 0, 0, 0, 0._plflt)
         endif
         call pltimefmt(time_format)
         call plbox("bcnstd", xlabel_step, 0, "bcnstv", 0._plflt, 0)
         call plcol0(3)
         title = "@frPLplot Example 29 - TAI-UTC "// &
             trim(title_suffix)
         call pllab(xtitle, "TAI-UTC (sec)", title)
    
         call plcol0(4)
         
         call plline(x(1:npts), y(1:npts))
      enddo
      end subroutine plot4