📄 sunriset.c
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/* +++Date last modified: 05-Jul-1997 */
/*
SUNRISET.C - computes Sun rise/set times, start/end of twilight, and
the length of the day at any date and latitude
Written as DAYLEN.C, 1989-08-16
Modified to SUNRISET.C, 1992-12-01
(c) Paul Schlyter, 1989, 1992
Released to the public domain by Paul Schlyter, December 1992
*/
#include <stdio.h>
#include <math.h>
/* A macro to compute the number of days elapsed since 2000 Jan 0.0 */
/* (which is equal to 1999 Dec 31, 0h UT) */
#define days_since_2000_Jan_0(y,m,d) \
(367L*(y)-((7*((y)+(((m)+9)/12)))/4)+((275*(m))/9)+(d)-730530L)
/* Some conversion factors between radians and degrees */
#ifndef PI
#define PI 3.1415926535897932384
#endif
#define RADEG ( 180.0 / PI )
#define DEGRAD ( PI / 180.0 )
/* The trigonometric functions in degrees */
#define sind(x) sin((x)*DEGRAD)
#define cosd(x) cos((x)*DEGRAD)
#define tand(x) tan((x)*DEGRAD)
#define atand(x) (RADEG*atan(x))
#define asind(x) (RADEG*asin(x))
#define acosd(x) (RADEG*acos(x))
#define atan2d(y,x) (RADEG*atan2(y,x))
/* Following are some macros around the "workhorse" function __daylen__ */
/* They mainly fill in the desired values for the reference altitude */
/* below the horizon, and also selects whether this altitude should */
/* refer to the Sun's center or its upper limb. */
/* This macro computes the length of the day, from sunrise to sunset. */
/* Sunrise/set is considered to occur when the Sun's upper limb is */
/* 35 arc minutes below the horizon (this accounts for the refraction */
/* of the Earth's atmosphere). */
#define day_length(year,month,day,lon,lat) \
__daylen__( year, month, day, lon, lat, -35.0/60.0, 1 )
/* This macro computes the length of the day, including civil twilight. */
/* Civil twilight starts/ends when the Sun's center is 6 degrees below */
/* the horizon. */
#define day_civil_twilight_length(year,month,day,lon,lat) \
__daylen__( year, month, day, lon, lat, -6.0, 0 )
/* This macro computes the length of the day, incl. nautical twilight. */
/* Nautical twilight starts/ends when the Sun's center is 12 degrees */
/* below the horizon. */
#define day_nautical_twilight_length(year,month,day,lon,lat) \
__daylen__( year, month, day, lon, lat, -12.0, 0 )
/* This macro computes the length of the day, incl. astronomical twilight. */
/* Astronomical twilight starts/ends when the Sun's center is 18 degrees */
/* below the horizon. */
#define day_astronomical_twilight_length(year,month,day,lon,lat) \
__daylen__( year, month, day, lon, lat, -18.0, 0 )
/* This macro computes times for sunrise/sunset. */
/* Sunrise/set is considered to occur when the Sun's upper limb is */
/* 35 arc minutes below the horizon (this accounts for the refraction */
/* of the Earth's atmosphere). */
#define sun_rise_set(year,month,day,lon,lat,rise,set) \
__sunriset__( year, month, day, lon, lat, -35.0/60.0, 1, rise, set )
/* This macro computes the start and end times of civil twilight. */
/* Civil twilight starts/ends when the Sun's center is 6 degrees below */
/* the horizon. */
#define civil_twilight(year,month,day,lon,lat,start,end) \
__sunriset__( year, month, day, lon, lat, -6.0, 0, start, end )
/* This macro computes the start and end times of nautical twilight. */
/* Nautical twilight starts/ends when the Sun's center is 12 degrees */
/* below the horizon. */
#define nautical_twilight(year,month,day,lon,lat,start,end) \
__sunriset__( year, month, day, lon, lat, -12.0, 0, start, end )
/* This macro computes the start and end times of astronomical twilight. */
/* Astronomical twilight starts/ends when the Sun's center is 18 degrees */
/* below the horizon. */
#define astronomical_twilight(year,month,day,lon,lat,start,end) \
__sunriset__( year, month, day, lon, lat, -18.0, 0, start, end )
/* Function prototypes */
double __daylen__( int year, int month, int day, double lon, double lat,
double altit, int upper_limb );
int __sunriset__( int year, int month, int day, double lon, double lat,
double altit, int upper_limb, double *rise, double *set );
void sunpos( double d, double *lon, double *r );
void sun_RA_dec( double d, double *RA, double *dec, double *r );
double revolution( double x );
double rev180( double x );
double GMST0( double d );
/* A small test program */
main()
{
int year,month,day;
double lon, lat;
double daylen, civlen, nautlen, astrlen;
double rise, set, civ_start, civ_end, naut_start, naut_end,
astr_start, astr_end;
int rs, civ, naut, astr;
char buf[80];
printf( "Longitude (+ is east) and latitude (+ is north) : " );
fgets(buf, 80, stdin);
sscanf(buf, "%lf %lf", &lon, &lat );
for(;;)
{
printf( "Input date ( yyyy mm dd ) (ctrl-C exits): " );
fgets(buf, 80, stdin);
sscanf(buf, "%d %d %d", &year, &month, &day );
daylen = day_length(year,month,day,lon,lat);
civlen = day_civil_twilight_length(year,month,day,lon,lat);
nautlen = day_nautical_twilight_length(year,month,day,lon,lat);
astrlen = day_astronomical_twilight_length(year,month,day,
lon,lat);
printf( "Day length: %5.2f hours\n", daylen );
printf( "With civil twilight %5.2f hours\n", civlen );
printf( "With nautical twilight %5.2f hours\n", nautlen );
printf( "With astronomical twilight %5.2f hours\n", astrlen );
printf( "Length of twilight: civil %5.2f hours\n",
(civlen-daylen)/2.0);
printf( " nautical %5.2f hours\n",
(nautlen-daylen)/2.0);
printf( " astronomical %5.2f hours\n",
(astrlen-daylen)/2.0);
rs = sun_rise_set ( year, month, day, lon, lat,
&rise, &set );
civ = civil_twilight ( year, month, day, lon, lat,
&civ_start, &civ_end );
naut = nautical_twilight ( year, month, day, lon, lat,
&naut_start, &naut_end );
astr = astronomical_twilight( year, month, day, lon, lat,
&astr_start, &astr_end );
printf( "Sun at south %5.2fh UT\n", (rise+set)/2.0 );
switch( rs )
{
case 0:
printf( "Sun rises %5.2fh UT, sets %5.2fh UT\n",
rise, set );
break;
case +1:
printf( "Sun above horizon\n" );
break;
case -1:
printf( "Sun below horizon\n" );
break;
}
switch( civ )
{
case 0:
printf( "Civil twilight starts %5.2fh, "
"ends %5.2fh UT\n", civ_start, civ_end );
break;
case +1:
printf( "Never darker than civil twilight\n" );
break;
case -1:
printf( "Never as bright as civil twilight\n" );
break;
}
switch( naut )
{
case 0:
printf( "Nautical twilight starts %5.2fh, "
"ends %5.2fh UT\n", naut_start, naut_end );
break;
case +1:
printf( "Never darker than nautical twilight\n" );
break;
case -1:
printf( "Never as bright as nautical twilight\n" );
break;
}
switch( astr )
{
case 0:
printf( "Astronomical twilight starts %5.2fh, "
"ends %5.2fh UT\n", astr_start, astr_end );
break;
case +1:
printf( "Never darker than astronomical twilight\n" );
break;
case -1:
printf( "Never as bright as astronomical twilight\n" );
break;
}
return 0;
}
}
/* The "workhorse" function for sun rise/set times */
int __sunriset__( int year, int month, int day, double lon, double lat,
double altit, int upper_limb, double *trise, double *tset )
/***************************************************************************/
/* Note: year,month,date = calendar date, 1801-2099 only. */
/* Eastern longitude positive, Western longitude negative */
/* Northern latitude positive, Southern latitude negative */
/* The longitude value IS critical in this function! */
/* altit = the altitude which the Sun should cross */
/* Set to -35/60 degrees for rise/set, -6 degrees */
/* for civil, -12 degrees for nautical and -18 */
/* degrees for astronomical twilight. */
/* upper_limb: non-zero -> upper limb, zero -> center */
/* Set to non-zero (e.g. 1) when computing rise/set */
/* times, and to zero when computing start/end of */
/* twilight. */
/* *rise = where to store the rise time */
/* *set = where to store the set time */
/* Both times are relative to the specified altitude, */
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