1 |
/*-------------------------------------------------------------------- |
2 |
* $Id: sun.c,v 1.6 2004/07/05 06:57:56 pa2h Exp $ |
3 |
* |
4 |
* This file is part of libRadtran. |
5 |
* Copyright (c) 1997-2001 by Arve Kylling and Bernhard Mayer. |
6 |
* |
7 |
* ######### Contact info: http://www.libradtran.org ######### |
8 |
* |
9 |
* This program is free software; you can redistribute it and/or |
10 |
* modify it under the terms of the GNU General Public License |
11 |
* as published by the Free Software Foundation; either version 2 |
12 |
* of the License, or (at your option) any later version. |
13 |
* |
14 |
* This program is distributed in the hope that it will be useful, |
15 |
* but WITHOUT ANY WARRANTY; without even the implied warranty of |
16 |
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the |
17 |
* GNU General Public License for more details. |
18 |
* |
19 |
* You should have received a copy of the GNU General Public License |
20 |
* along with this program; if not, write to the Free Software |
21 |
* Foundation, Inc., 59 Temple Place - Suite 330, |
22 |
* Boston, MA 02111-1307, USA. |
23 |
*--------------------------------------------------------------------*/ |
24 |
|
25 |
|
26 |
/* sun.a - Solar zenith and azimuth calculations @ti@ */ |
27 |
/* */ |
28 |
/* Most of the formulas are adopted from: */ |
29 |
/* Iqbal, Muhammad: "An Introduction to Solar Radiation", */ |
30 |
/* Academic Press, Inc., 1983 */ |
31 |
/* (page numbers in the comments refer to this book). */ |
32 |
/* */ |
33 |
/* Time is specified in seconds from midnight, */ |
34 |
/* angles are specified in degrees. */ |
35 |
|
36 |
#include <math.h> |
37 |
#include <stdio.h> |
38 |
#include <string.h> |
39 |
#include "sun.h" |
40 |
|
41 |
|
42 |
|
43 |
/* @42c@ */ |
44 |
/* @c42@ */ |
45 |
/****************************************************************************/ |
46 |
/* In order to use the functions provided by the sun library, @42_10c@ */ |
47 |
/* #include <sun.h> in your source code and link with libRadtran_c.a. */ |
48 |
/* */ |
49 |
/* @strong{Example:} */ |
50 |
/* Example for a source file: */ |
51 |
/* @example */ |
52 |
/* */ |
53 |
/* ... */ |
54 |
/* #include "../src_c/sun.h" */ |
55 |
/* ... */ |
56 |
/* */ |
57 |
/* @end example */ |
58 |
/* */ |
59 |
/* Linking of the executable, using the GNU compiler gcc: */ |
60 |
/* @example */ |
61 |
/* */ |
62 |
/* gcc -o test test.c -lRadtran_c -L../lib */ |
63 |
/* */ |
64 |
/* @end example @c42_10@ */ |
65 |
/****************************************************************************/ |
66 |
|
67 |
|
68 |
/****************************************************************************/ |
69 |
/* The sun library provides functions for solar zenith and azimuth @42_20c@ */ |
70 |
/* angle and sun-earth-distance calculations. All formulas have been taken */ |
71 |
/* from Iqbal, "An introduction to solar radiation". */ |
72 |
/* @c42_20@ */ |
73 |
/****************************************************************************/ |
74 |
|
75 |
|
76 |
/* define _PI_ */ |
77 |
#define _PI_ 3.1415926 |
78 |
|
79 |
/* internal functions */ |
80 |
static double dayangle (int day); |
81 |
|
82 |
|
83 |
/***********************************************************************************/ |
84 |
/* Function: dayangle */ |
85 |
/* Description: */ |
86 |
/* Internal function to calculate the dayangle according to Iqbal, pg. 3 */ |
87 |
/* */ |
88 |
/* Parameters: */ |
89 |
/* int day: day of year. */ |
90 |
/* */ |
91 |
/* Return value: */ |
92 |
/* double dayangle, 0..2pi */ |
93 |
/* */ |
94 |
/* Example: */ |
95 |
/* Files: */ |
96 |
/* Known bugs: */ |
97 |
/* Author: */ |
98 |
/* */ |
99 |
/***********************************************************************************/ |
100 |
|
101 |
static double dayangle (int day) |
102 |
{ |
103 |
return 2.0 * _PI_ * (double) (day-1) / 365.0; |
104 |
} |
105 |
|
106 |
|
107 |
|
108 |
/***********************************************************************************/ |
109 |
/* Function: eccentricity @42_30i@ */ |
110 |
/* Description: */ |
111 |
/* Calculate the eccentricity correction factor E0 = (r0/r)**2 according to */ |
112 |
/* Iqbal, page 3. This factor, when multiplied with the irradiance, accounts */ |
113 |
/* for the annual variation of the sun-earth-distance. */ |
114 |
/* */ |
115 |
/* Parameters: */ |
116 |
/* int day: day of year (leap day is usually @strong{not} counted. */ |
117 |
/* */ |
118 |
/* Return value: */ |
119 |
/* The eccentricity (double) for the specified day. */ |
120 |
/* */ |
121 |
/* Example: */ |
122 |
/* Files: */ |
123 |
/* Known bugs: */ |
124 |
/* Author: */ |
125 |
/* @i42_30@ */ |
126 |
/***********************************************************************************/ |
127 |
|
128 |
double eccentricity (int day) |
129 |
{ |
130 |
double E0=0, angle=0; |
131 |
|
132 |
angle = dayangle (day); |
133 |
|
134 |
E0 = 1.000110 + 0.034221 * cos(angle) + 0.001280 * sin(angle) |
135 |
+ 0.000719 * cos(2*angle) + 0.000077 * sin(2*angle); |
136 |
|
137 |
return E0; |
138 |
} |
139 |
|
140 |
|
141 |
|
142 |
/***********************************************************************************/ |
143 |
/* Function: declination @42_30i@ */ |
144 |
/* Description: */ |
145 |
/* Calculate the declination for a specified day (Iqbal, page 7). */ |
146 |
/* */ |
147 |
/* Parameters: */ |
148 |
/* int day: day of year (leap day is usually @strong{not} counted. */ |
149 |
/* */ |
150 |
/* Return value: */ |
151 |
/* The declination in degrees (double) for the specified day. */ |
152 |
/* */ |
153 |
/* Example: */ |
154 |
/* Files: */ |
155 |
/* Known bugs: */ |
156 |
/* Author: */ |
157 |
/* @i42_30@ */ |
158 |
/***********************************************************************************/ |
159 |
|
160 |
double declination (int day) |
161 |
{ |
162 |
double delta=0, angle=0; |
163 |
|
164 |
angle = dayangle (day); |
165 |
|
166 |
delta = 0.006918 - 0.399912 * cos (angle) + 0.070257 * sin (angle) |
167 |
- 0.006758 * cos (2*angle) + 0.000907 * sin (2*angle) |
168 |
- 0.002697 * cos (3*angle) + 0.00148 * sin (3*angle); |
169 |
|
170 |
delta *= 180.0/_PI_; |
171 |
|
172 |
return delta; |
173 |
} |
174 |
|
175 |
|
176 |
|
177 |
/***********************************************************************************/ |
178 |
/* Function: equation_of_time @42_30i@ */ |
179 |
/* Description: */ |
180 |
/* Calculate the equation of time for a specified day (Iqbal, page 11). */ |
181 |
/* */ |
182 |
/* Parameters: */ |
183 |
/* int day: day of year (leap day is usually @strong{not} counted. */ |
184 |
/* */ |
185 |
/* Return value: */ |
186 |
/* The equation of time in seconds (double) for the specified day. */ |
187 |
/* */ |
188 |
/* Example: */ |
189 |
/* Files: */ |
190 |
/* Known bugs: */ |
191 |
/* Author: */ |
192 |
/* @i42_30@ */ |
193 |
/***********************************************************************************/ |
194 |
|
195 |
int equation_of_time (int day) |
196 |
{ |
197 |
double angle=0, et=0; |
198 |
|
199 |
angle = dayangle (day); |
200 |
|
201 |
et = (0.000075 + 0.001868 * cos(angle) - 0.032077 * sin(angle) |
202 |
-0.014615 * cos(2*angle) - 0.04089 * sin(2*angle)) * 13750.8; |
203 |
|
204 |
return (int) (et+0.5); |
205 |
} |
206 |
|
207 |
|
208 |
|
209 |
/***********************************************************************************/ |
210 |
/* Function: LAT @42_30i@ */ |
211 |
/* Description: */ |
212 |
/* Calculate the local apparent time for a given standard time and location. */ |
213 |
/* */ |
214 |
/* Parameters: */ |
215 |
/* int time_std: Standard time [seconds since midnight]. */ |
216 |
/* int day: day of year (leap day is usually @strong{not} counted. */ |
217 |
/* double longitude: Longitude [degrees] (West positive). */ |
218 |
/* double long_std: Standard longitude [degrees]. */ |
219 |
/* */ |
220 |
/* Return value: */ |
221 |
/* The local apparent time in seconds since midnight (double). */ |
222 |
/* */ |
223 |
/* Example: */ |
224 |
/* Files: */ |
225 |
/* Known bugs: */ |
226 |
/* Author: */ |
227 |
/* @i42_30@ */ |
228 |
/***********************************************************************************/ |
229 |
|
230 |
int LAT (int time_std, int day, double longitude, double long_std) |
231 |
{ |
232 |
int lat=0; |
233 |
|
234 |
lat = time_std + (int) (240.0 * (long_std-longitude)) |
235 |
+ equation_of_time (day); |
236 |
|
237 |
return lat; |
238 |
} |
239 |
|
240 |
|
241 |
/************************************************/ |
242 |
/* convert local apparent time to standard time */ |
243 |
/************************************************/ |
244 |
|
245 |
int standard_time (int lat, int day, double longitude, double long_std) |
246 |
{ |
247 |
return lat - (int) (240.0 * (long_std-longitude)) - equation_of_time (day); |
248 |
} |
249 |
|
250 |
|
251 |
/****************************/ |
252 |
/* hour angle omega; pg. 15 */ |
253 |
/****************************/ |
254 |
|
255 |
double hour_angle (int time) |
256 |
{ |
257 |
double omega=0; |
258 |
|
259 |
omega = _PI_ * (1.0 - ((double) time) / 43200.0); |
260 |
|
261 |
omega *= 180.0/_PI_; |
262 |
return omega; |
263 |
} |
264 |
|
265 |
|
266 |
|
267 |
/***********************************************************************************/ |
268 |
/* Function: solar_zenith @42_30i@ */ |
269 |
/* Description: */ |
270 |
/* Calculate the solar zenith angle for a given time and location. */ |
271 |
/* */ |
272 |
/* Parameters: */ |
273 |
/* int time: Standard time [seconds since midnight]. */ |
274 |
/* int day: day of year (leap day is usually @strong{not} counted. */ |
275 |
/* double latitude: Latitude [degrees] (North positive). */ |
276 |
/* double longitude: Longitude [degrees] (West positive). */ |
277 |
/* double long_std: Standard longitude [degrees]. */ |
278 |
/* */ |
279 |
/* Return value: */ |
280 |
/* The solar zenith angle [degrees]. */ |
281 |
/* */ |
282 |
/* Example: */ |
283 |
/* Files: */ |
284 |
/* Known bugs: */ |
285 |
/* Author: */ |
286 |
/* @i42_30@ */ |
287 |
/***********************************************************************************/ |
288 |
|
289 |
double solar_zenith (int time, int day, |
290 |
double latitude, double longitude, double long_std) |
291 |
{ |
292 |
double theta=0, omega=0, delta=0, phi = latitude*_PI_/180.0; |
293 |
int lat = LAT (time, day, longitude, long_std); |
294 |
|
295 |
delta = _PI_/180.0*declination (day); |
296 |
omega = _PI_/180.0*hour_angle (lat); |
297 |
|
298 |
theta = acos(sin(delta) * sin(phi) + cos(delta) * cos(phi) * cos(omega)); |
299 |
|
300 |
theta *= (180.0/_PI_); /* convert to degrees */ |
301 |
return theta; |
302 |
} |
303 |
|
304 |
|
305 |
|
306 |
|
307 |
/***********************************************************************************/ |
308 |
/* Function: solar_azimuth @42_30i@ */ |
309 |
/* Description: */ |
310 |
/* Calculate the solar azimuth angle for a given time and location. */ |
311 |
/* */ |
312 |
/* Parameters: */ |
313 |
/* int time: Standard time [seconds since midnight]. */ |
314 |
/* int day: day of year (leap day is usually @strong{not} counted. */ |
315 |
/* double latitude: Latitude [degrees] (North positive). */ |
316 |
/* double longitude: Longitude [degrees] (West positive). */ |
317 |
/* double long_std: Standard longitude [degrees]. */ |
318 |
/* */ |
319 |
/* Return value: */ |
320 |
/* The solar azimuth angle [degrees]. */ |
321 |
/* */ |
322 |
/* Example: */ |
323 |
/* Files: */ |
324 |
/* Known bugs: */ |
325 |
/* Author: */ |
326 |
/* @i42_30@ */ |
327 |
/***********************************************************************************/ |
328 |
|
329 |
double solar_azimuth (int time, int day, |
330 |
double latitude, double longitude, double long_std) |
331 |
{ |
332 |
double theta=0, omega=0, delta=0, phi = latitude*_PI_/180.0, psi=0, cospsi=0; |
333 |
int lat = LAT (time, day, longitude, long_std); |
334 |
|
335 |
delta = _PI_/180.0*declination (day); |
336 |
omega = _PI_/180.0*hour_angle (lat); |
337 |
theta = _PI_/180.0*solar_zenith (time, day, latitude, longitude, long_std); |
338 |
|
339 |
|
340 |
cospsi = (cos(theta)*sin(phi) - sin(delta)) / sin(theta) / cos (phi); |
341 |
/* allow tiny roundoff errors */ |
342 |
if (cospsi>1.0 && cospsi<1.0+1e-6) |
343 |
cospsi=1.0; |
344 |
|
345 |
if (cospsi<-1.0 && cospsi>-1.0-1e-6) |
346 |
cospsi=-1.0; |
347 |
|
348 |
psi = -acos(cospsi); |
349 |
|
350 |
/* adjust sign */ |
351 |
if (lat>43200 || lat<0) |
352 |
psi=-psi; |
353 |
|
354 |
psi *= (180.0/_PI_); /* convert to degrees */ |
355 |
|
356 |
return psi; |
357 |
} |
358 |
|
359 |
|
360 |
|
361 |
/***********************************************************************************/ |
362 |
/* Function: day_of_year @42_30i@ */ |
363 |
/* Description: */ |
364 |
/* Calculate the day of year for given date (leap days are not considered. */ |
365 |
/* */ |
366 |
/* Parameters: */ |
367 |
/* int day: Day of month (1..31). */ |
368 |
/* int month: Month (1..12). */ |
369 |
/* */ |
370 |
/* Return value: */ |
371 |
/* The day of year (int); -1 if error. */ |
372 |
/* */ |
373 |
/* Example: */ |
374 |
/* Files: */ |
375 |
/* Known bugs: */ |
376 |
/* Author: */ |
377 |
/* @i42_30@ */ |
378 |
/***********************************************************************************/ |
379 |
|
380 |
int day_of_year (int day, int month) |
381 |
{ |
382 |
char mon = 0; |
383 |
int doy = -1; |
384 |
|
385 |
if (month<1 || month > 12) |
386 |
return (-1); |
387 |
|
388 |
if (day<1 || day > 31) |
389 |
return (-1); |
390 |
|
391 |
mon = (char) month; |
392 |
|
393 |
switch (mon) { |
394 |
case 1: |
395 |
doy = day + 0; |
396 |
break; |
397 |
case 2: |
398 |
doy = day + 31; |
399 |
break; |
400 |
case 3: |
401 |
doy = day + 59; |
402 |
break; |
403 |
case 4: |
404 |
doy = day + 90; |
405 |
break; |
406 |
case 5: |
407 |
doy = day + 120; |
408 |
break; |
409 |
case 6: |
410 |
doy = day + 151; |
411 |
break; |
412 |
case 7: |
413 |
doy = day + 181; |
414 |
break; |
415 |
case 8: |
416 |
doy = day + 212; |
417 |
break; |
418 |
case 9: |
419 |
doy = day + 243; |
420 |
break; |
421 |
case 10: |
422 |
doy = day + 273; |
423 |
break; |
424 |
case 11: |
425 |
doy = day + 304; |
426 |
break; |
427 |
case 12: |
428 |
doy = day + 334; |
429 |
break; |
430 |
default: |
431 |
doy = -1; |
432 |
} |
433 |
|
434 |
return (doy); |
435 |
} |
436 |
|
437 |
|
438 |
|
439 |
|
440 |
/**************************************************************************/ |
441 |
/* convert time to string */ |
442 |
/* memory for timestr must be allocated by programmer (at least 10 bytes) */ |
443 |
/**************************************************************************/ |
444 |
|
445 |
char *time2str (char *timestr, int hour, int min, int sec) |
446 |
{ |
447 |
char hourstr[3] = ""; |
448 |
char minstr[3] = ""; |
449 |
char secstr[3] = ""; |
450 |
|
451 |
strcpy (timestr, ""); |
452 |
|
453 |
if (hour<0 || hour>24) |
454 |
return NULL; |
455 |
|
456 |
if (min<0 || min>60) |
457 |
return NULL; |
458 |
|
459 |
if (sec<0 || sec>60) |
460 |
return NULL; |
461 |
|
462 |
|
463 |
|
464 |
if (hour<10) |
465 |
sprintf (hourstr, "0%d", hour); |
466 |
else |
467 |
sprintf (hourstr, "%d", hour); |
468 |
|
469 |
if (min<10) |
470 |
sprintf (minstr, "0%d", min); |
471 |
else |
472 |
sprintf (minstr, "%d", min); |
473 |
|
474 |
if (sec<10) |
475 |
sprintf (secstr, "0%d", sec); |
476 |
else |
477 |
sprintf (secstr, "%d", sec); |
478 |
|
479 |
sprintf (timestr, "%s:%s:%s", hourstr, minstr, secstr); |
480 |
|
481 |
return timestr; |
482 |
} |
483 |
|
484 |
|
485 |
|
486 |
|
487 |
/***********************************************************************************/ |
488 |
/* Function: zenith2time @42_30i@ */ |
489 |
/* Description: */ |
490 |
/* Calculate the times for a given solar zenith angle, day of year and location. */ |
491 |
/* */ |
492 |
/* Parameters: */ |
493 |
/* int day: day of year */ |
494 |
/* double zenith_angle: Solar zenith angle [degrees]. */ |
495 |
/* double latitude: Latitude [degrees] (North positive). */ |
496 |
/* double longitude: Longitude [degrees] (West positive). */ |
497 |
/* double long_std: Standard longitude [degrees]. */ |
498 |
/* int *time1: 1st time of occurence. */ |
499 |
/* int *time2: 2nd time of occurence. */ |
500 |
/* */ |
501 |
/* Return value: */ |
502 |
/* 0 if o.k., <0 if error. */ |
503 |
/* */ |
504 |
/* Example: */ |
505 |
/* Files: */ |
506 |
/* Known bugs: */ |
507 |
/* Author: */ |
508 |
/* @i42_30@ */ |
509 |
/***********************************************************************************/ |
510 |
|
511 |
int zenith2time (int day, |
512 |
double zenith_angle, |
513 |
double latitude, |
514 |
double longitude, |
515 |
double long_std, |
516 |
int *time1, |
517 |
int *time2) |
518 |
{ |
519 |
double delta = _PI_/180.0*declination (day); |
520 |
double phi = _PI_/180.0*latitude; |
521 |
double theta = _PI_/180.0*zenith_angle; |
522 |
double cos_omega = (cos(theta) - sin(delta)*sin(phi)) / |
523 |
cos(delta) / cos(phi); |
524 |
double omega1=0, omega2=0; |
525 |
int lat1=0, lat2=0; |
526 |
|
527 |
if (fabs(cos_omega) > 1.0) |
528 |
return ERROR_NO_ZENITH; |
529 |
|
530 |
omega1 = acos (cos_omega); |
531 |
omega2 = 0.0-omega1; |
532 |
|
533 |
lat1 = 43200*(1-omega1/_PI_); |
534 |
lat2 = 43200*(1-omega2/_PI_); |
535 |
|
536 |
*time1 = standard_time (lat1, day, longitude, long_std); |
537 |
*time2 = standard_time (lat2, day, longitude, long_std); |
538 |
|
539 |
return 0; |
540 |
} |
541 |
|
542 |
|
543 |
|
544 |
|
545 |
|
546 |
/***********************************************************************************/ |
547 |
/* Function: Gregorian2Julian @42_30i@ */ |
548 |
/* Description: */ |
549 |
/* Convert from Gregorian day (day, month, year) to Julian day (by the */ |
550 |
/* astronomical definition). This function, in combination with */ |
551 |
/* Julian2Gregorian() is very useful to answer questions like "which date is */ |
552 |
/* 666 days after December 31, 1999?" Algorithm from */ |
553 |
/* H.F. Fliegel and T.C. Van Flandern, "A Machine Algorithm for Processing */ |
554 |
/* Calendar Dates", Communications of the Association for Computing Machinery */ |
555 |
/* (CACM), Vol. 11, No. 10, 657, 1968. */ |
556 |
/* */ |
557 |
/* Parameters: */ |
558 |
/* int d: Day of month (1..31). */ |
559 |
/* int m: Month (1..12). */ |
560 |
/* int y: Year (attention: full year required, 1999 instead of 99) */ |
561 |
/* int *jd: The Julian day, to be calculated. */ |
562 |
/* */ |
563 |
/* Return value: */ |
564 |
/* 0 if o.k., <0 if error. */ |
565 |
/* */ |
566 |
/* Example: */ |
567 |
/* Files: */ |
568 |
/* Known bugs: */ |
569 |
/* Author: */ |
570 |
/* @i42_30@ */ |
571 |
/***********************************************************************************/ |
572 |
|
573 |
int Gregorian2Julian (int d, int m, int y, int *jd) |
574 |
{ |
575 |
char ystr[3]=""; |
576 |
|
577 |
/* reset output */ |
578 |
*jd =0; |
579 |
|
580 |
if (d<1||d>31) |
581 |
return -1; |
582 |
|
583 |
if (m<1||m>12) |
584 |
return -1; |
585 |
|
586 |
if (y>0&&y<100) { |
587 |
if (y<10) |
588 |
sprintf (ystr, "0%d", y); |
589 |
else |
590 |
sprintf (ystr, "%d", y); |
591 |
|
592 |
fprintf (stderr, "Warning: Gregorian2Julian() has been called for year %s\n", ystr); |
593 |
fprintf (stderr, "Maybe you meant 19%s or 20%s?\n", ystr, ystr); |
594 |
} |
595 |
|
596 |
|
597 |
*jd = (1461 * (y + 4800 + (m - 14) / 12)) / 4 + |
598 |
(367 * (m - 2 - 12 * ((m - 14) / 12))) / 12 - |
599 |
(3 * ((y + 4900 + (m - 14) / 12) / 100)) / 4 + d - 32075; |
600 |
|
601 |
return 0; /* if o.k. */ |
602 |
} |
603 |
|
604 |
|
605 |
|
606 |
/***********************************************************************************/ |
607 |
/* Function: Julian2Gregorian @42_30i@ */ |
608 |
/* Description: */ |
609 |
/* Convert from Julian day (by the astronomical definition) to Gregorian day */ |
610 |
/* (day, month, year) to . This function, in combination with */ |
611 |
/* Gregorian2Julian() is very useful to answer questions like "which date is */ |
612 |
/* 666 days after December 31, 1999?" Algorithm from */ |
613 |
/* H.F. Fliegel and T.C. Van Flandern, "A Machine Algorithm for Processing */ |
614 |
/* Calendar Dates", Communications of the Association for Computing Machinery */ |
615 |
/* (CACM), Vol. 11, No. 10, 657, 1968. */ |
616 |
/* */ |
617 |
/* Parameters: */ |
618 |
/* int *d: Day of month (1..31), to be calculated. */ |
619 |
/* int *m: Month (1..12), to be calculated. */ |
620 |
/* int *y: Year, to be calculated. */ |
621 |
/* int jd: The Julian day. */ |
622 |
/* */ |
623 |
/* Return value: */ |
624 |
/* 0 if o.k., <0 if error. */ |
625 |
/* */ |
626 |
/* Example: */ |
627 |
/* Files: */ |
628 |
/* Known bugs: */ |
629 |
/* Author: */ |
630 |
/* @i42_30@ */ |
631 |
/***********************************************************************************/ |
632 |
|
633 |
int Julian2Gregorian(int *d, int *m, int *y, int jd) |
634 |
{ |
635 |
int l=0, n=0, i=0, j=0; |
636 |
|
637 |
l = jd + 68569; |
638 |
n = ( 4 * l ) / 146097; |
639 |
l = l - ( 146097 * n + 3 ) / 4; |
640 |
i = ( 4000 * ( l + 1 ) ) / 1461001; |
641 |
l = l - ( 1461 * i ) / 4 + 31; |
642 |
j = ( 80 * l ) / 2447; |
643 |
*d = l - ( 2447 * j ) / 80; |
644 |
l = j / 11; |
645 |
*m = j + 2 - ( 12 * l ); |
646 |
*y = 100 * ( n - 49 ) + i + l; |
647 |
|
648 |
return 0; |
649 |
} |
650 |
|
651 |
|
652 |
/***********************************************************************************/ |
653 |
/* Function: location @42_30i@ */ |
654 |
/* Description: */ |
655 |
/* Return latitude, longitude, and standard longitude for a given location. */ |
656 |
/* */ |
657 |
/* Parameters: */ |
658 |
/* double *latitude: Latitude (North positive). */ |
659 |
/* double *longitude: Longitude (West positive). */ |
660 |
/* double *long_std: Standard longitude (West positive). */ |
661 |
/* char *location: String identifying the location. */ |
662 |
/* */ |
663 |
/* Return value: */ |
664 |
/* 0 if o.k., <0 if error. */ |
665 |
/* */ |
666 |
/* Example: */ |
667 |
/* Files: */ |
668 |
/* Known bugs: */ |
669 |
/* Author: */ |
670 |
/* @i42_30@ */ |
671 |
/***********************************************************************************/ |
672 |
|
673 |
int location (char *locstr, double *latitude, double *longitude, double *long_std) |
674 |
{ |
675 |
|
676 |
if (!strcasecmp(locstr, "ifu")) { |
677 |
*latitude = 47.48; |
678 |
*longitude = -11.07; |
679 |
*long_std = -15.00; |
680 |
|
681 |
return 0; |
682 |
} |
683 |
|
684 |
if (!strcasecmp(locstr, "dlrop")) { |
685 |
*latitude = 48.088; |
686 |
*longitude = -11.280; |
687 |
*long_std = -15.000; |
688 |
|
689 |
return 0; |
690 |
} |
691 |
|
692 |
|
693 |
return -1; |
694 |
} |