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skycalendar.c
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skycalendar.c
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/*
This is a self-contained c-language program to print a nighttime
astronomical calendar for use in planning observations.
It prints to standard output (usually the terminal); the
operator should capture this output (e. g., using redirection
in UNIX or the /out= switch in VMS) and then print it on an
appropriate output device. The table which is printed is some
125 columns wide, so a wide device is required (either a line
printer or a laserprinter in LANDSCAPE mode.) It is assumed that
the ASCII form-feed character will actually begin a new page.
The original program was to run on VMS, but it should be very
transportable. Non-vms users will probably want to change
'unixio.h' to 'stdio.h' in the first line.
An explanatory text is printed at the beginning of the output, which
includes the appropriate CAUTIONS regarding accuracy and applicability.
A number of 'canned site' parameters have been included. Be
careful of time zones, DST etc. for foreign sites.
To customize to your own site, install an option in the
routine 'load_site'. The code is very straightforward; just do
it exactly the same as the others. You might also want to erase
some seldom-used choices. One can also specify new site parameters
at run time.
This program may be used freely by anyone for scientific or educational
purposes. If you use it for profit, I want a cut, and claim
a copyright herewith. In any case please acknowledge the source:
John Thorstensen
Dept. of Physics and Astronomy
Dartmouth College
Hanover, NH 03755
May 26, 1993.
*/
#include <stdio.h>
#include <math.h>
double pi = 3.14159265358979;
#define PI 3.14159265358979
#define ARCSEC_IN_RADIAN 206264.8062
#define DEG_IN_RADIAN 57.2957795130823
#define HRS_IN_RADIAN 3.819718634
#define J2000 2451545.
#define SEC_IN_DAY 86400.
#define FLATTEN 0.003352813
#define EQUAT_RAD 6378137.
#define TWILIGHT_ALT -18.
struct coord
{
short sign; /* carry sign explicitly since -0 not neg. */
double hh;
double mm;
double ss;
};
struct coord_pair
{
struct coord RA;
struct coord dec;
};
double bab_to_dec (bab)
struct coord bab;
{
double x;
x = bab.sign * (bab.hh + bab.mm / 60. + bab.ss / 3600.);
return(x);
}
void dec_to_bab (deci,bab)
/* function for converting decimal to babylonian hh mm ss.ss */
double deci;
struct coord *bab;
{
int hr_int, min_int;
if (deci >= 0.) bab->sign = 1;
else {
bab->sign = -1;
deci = -1. * deci;
}
hr_int = deci; /* use conversion conventions to truncate */
bab->hh = hr_int;
min_int = 60. * (deci - bab->hh);
bab->mm = min_int;
bab->ss = 3600. * (deci - bab->hh - bab->mm / 60.);
}
double get_coord()
/* Reads a string from the terminal and converts it into
a double-precision coordinate. This is trickier than
it appeared at first, since a -00 tests as non-negative;
the sign has to be picked out and handled explicitly. */
/* Prompt for input in the calling routine.*/
{
short sign;
double hrs, mins, secs;
char hh_string[6]; /* string with the first coord (hh) */
char hh1[1];
short i = 0;
/* read and handle the hour (or degree) part with sign */
scanf("%s",hh_string);
hh1[0] = hh_string[i];
while(hh1[0] == ' ') {
/* discard leading blanks */
i++;
hh1[0] = hh_string[i];
}
if(hh1[0] == '-') sign = -1;
else sign = 1;
sscanf(hh_string,"%lf", &hrs);
if(sign == -1) hrs = -1. * hrs;
/* read in the minutes and seconds normally */
scanf("%lf %lf",&mins,&secs);
return(sign * (hrs + mins / 60. + secs / 3600.));
}
void put_coords(deci, precision)
double deci; /* decimal coordinate */
short precision;
/* prints out a struct coord in a nice format; precision
is a code for how accurate you want it. The options are:
precision = 0; minutes rounded to the nearest minute
precision = 1; minutes rounded to the nearest tenth.
precision = 2; seconds rounded to the nearest second
precision = 3; seconds given to the tenth
precision = 4; seconds given to the hundredth
The program assumes that the line is ready for the coord
to be printed and does NOT deliver a new line at the end
of the output. */
{
double minutes; /* for rounding off if necess. */
struct coord out_coord, coords;
char out_string[20]; /* for checking for nasty 60's */
dec_to_bab(deci,&coords); /* internally convert to coords*/
if(coords.sign == -1) printf("-");
else printf(" "); /* to preserve alignment */
if(precision == 0) { /* round to nearest minute */
minutes = coords.mm + coords.ss / 60.;
/* check to be sure minutes aren't 60 */
sprintf(out_string,"%.0f %02.0f",coords.hh,minutes);
sscanf(out_string,"%lf %lf",&out_coord.hh,&out_coord.mm);
if(fabs(out_coord.mm - 60.) < 1.0e-7) {
out_coord.mm = 0.;
out_coord.hh = out_coord.hh + 1.;
}
printf("%2.0f %02.0f",out_coord.hh,out_coord.mm);
}
else if(precision == 1) { /* keep nearest tenth of a minute */
minutes = coords.mm + coords.ss / 60.;
/* check to be sure minutes are not 60 */
sprintf(out_string,"%.0f %04.1f",coords.hh,minutes);
sscanf(out_string,"%lf %lf",&out_coord.hh, &out_coord.mm);
if(fabs(out_coord.mm - 60.) < 1.0e-7) {
out_coord.mm = 0.;
out_coord.hh = out_coord.hh + 1.;
}
printf("%2.0f %04.1f", out_coord.hh, out_coord.mm);
}
else if(precision == 2) {
/* check to be sure seconds are not 60 */
sprintf(out_string,"%.0f %02.0f %02.0f",coords.hh,coords.mm,coords.ss);
sscanf(out_string,"%lf %lf %lf",&out_coord.hh,&out_coord.mm,
&out_coord.ss);
if(fabs(out_coord.ss - 60.) < 1.0e-7) {
out_coord.mm = out_coord.mm + 1.;
out_coord.ss = 0.;
if(fabs(out_coord.mm - 60.) < 1.0e-7) {
out_coord.hh = out_coord.hh + 1.;
out_coord.mm = 0.;
}
}
printf("%2.0f %02.0f %02.0f",out_coord.hh,out_coord.mm,out_coord.ss);
}
else if(precision == 3) {
/* the usual shuffle to check for 60's */
sprintf(out_string,"%.0f %02.0f %04.1f",coords.hh, coords.mm, coords.ss);
sscanf(out_string,"%lf %lf %lf",&out_coord.hh,&out_coord.mm,
&out_coord.ss);
if(fabs(out_coord.ss - 60.) < 1.0e-7) {
out_coord.mm = out_coord.mm + 1.;
out_coord.ss = 0.;
if(fabs(out_coord.mm - 60.) < 1.0e-7) {
out_coord.hh = out_coord.hh + 1.;
out_coord.mm = 0.;
}
}
printf("%2.0f %02.0f %04.1f",out_coord.hh,out_coord.mm,out_coord.ss);
}
else {
sprintf(out_string,"%.0f %02.0f %05.2f",coords.hh,coords.mm,coords.ss);
sscanf(out_string,"%lf %lf %lf",&out_coord.hh,&out_coord.mm,
&out_coord.ss);
if(fabs(out_coord.ss - 60.) < 1.0e-6) {
out_coord.mm = out_coord.mm + 1.;
out_coord.ss = 0.;
if(fabs(out_coord.mm - 60.) < 1.0e-6) {
out_coord.hh = out_coord.hh + 1.;
out_coord.mm = 0.;
}
}
printf("%2.0f %02.0f %05.2f",out_coord.hh, out_coord.mm, out_coord.ss);
}
}
double atan_circ(x,y)
double x, y;
{
/* returns radian angle 0 to 2pi for coords x, y */
double theta;
if(x == 0) {
if(y > 0.) theta = PI/2.;
else if(y < 0.) theta = 3.*PI/2.;
else theta = 0.; /* x and y zero */
}
else theta = atan(y/x);
if(x < 0.) theta = theta + PI;
if(theta < 0.) theta = theta + 2.*PI;
return(theta);
}
double altit(dec,ha,lat)
double dec,ha,lat; /* dec deg, dec hrs, dec deg */
{
double x;
dec = dec / DEG_IN_RADIAN;
ha = ha / HRS_IN_RADIAN;
lat = lat / DEG_IN_RADIAN; /* thank heavens for pass-by-value */
x = DEG_IN_RADIAN * asin(cos(dec)*cos(ha)*cos(lat) + sin(dec)*sin(lat));
return(x);
}
void min_max_alt(lat,dec,min,max)
double lat, dec, *min, *max;
{
/* computes minimum and maximum altitude for a given dec and
latitude. */
double x;
lat = lat / DEG_IN_RADIAN; /* pass by value! */
dec = dec / DEG_IN_RADIAN;
x = cos(dec)*cos(lat) + sin(dec)*sin(lat);
if(fabs(x) <= 1.) {
*max = asin(x) * DEG_IN_RADIAN;
}
else printf("Error in min_max_alt -- arcsin(>1)\n");
x = sin(dec)*sin(lat) - cos(dec)*cos(lat);
if(fabs(x) <= 1.) {
*min = asin(x) * DEG_IN_RADIAN;
}
else printf("Error in min_max_alt -- arcsin(>1)\n");
}
double ha_alt(dec,lat,alt)
double dec,lat,alt; /* dec deg */
{
/* returns hour angle at which object at dec is at altitude alt */
double x,coalt,min,max;
min_max_alt(lat,dec,&min,&max);
if(alt < min)
return(1000.); /* flag value - always higher than asked */
if(alt > max)
return(-1000.); /* flag for object always lower than asked */
dec = (0.5*PI) - dec / DEG_IN_RADIAN;
lat = (0.5*PI) - lat / DEG_IN_RADIAN;
coalt = (0.5*PI) - alt / DEG_IN_RADIAN;
x = (cos(coalt) - cos(dec)*cos(lat)) / (sin(dec)*sin(lat));
if(fabs(x) <= 1.) return(acos(x) * HRS_IN_RADIAN);
else {
printf("Error in ha_alt ... acos(>1).\n");
return(1000.);
}
}
double subtend(ra1,dec1,ra2,dec2)
double ra1, dec1, ra2, dec2; /* dec hrs and dec degrees */
{
/* angle subtended by two directions in the sky. */
double x1, y1, z1, x2, y2, z2;
double theta;
ra1 = ra1 / HRS_IN_RADIAN;
dec1 = dec1 / DEG_IN_RADIAN;
ra2 = ra2 / HRS_IN_RADIAN;
dec2 = dec2 / DEG_IN_RADIAN;
x1 = cos(ra1)*cos(dec1);
y1 = sin(ra1)*cos(dec1);
z1 = sin(dec1);
x2 = cos(ra2)*cos(dec2);
y2 = sin(ra2)*cos(dec2);
z2 = sin(dec2);
theta = acos(x1*x2+y1*y2+z1*z2);
return(theta);
}
struct date_time
{
short y;
short mo;
short d;
short h;
short mn;
float s;
};
double date_to_jd(date)
struct date_time date;
{
short yr1=0, mo1=1;
long jdzpt = 1720982, jdint, inter;
double jd,jdfrac;
if((date.y <= 1900) | (date.y >= 2100)) {
printf("Date out of range. 1900 - 2100 only.\n");
return(0.);
}
if(date.mo <= 2) {
yr1 = -1;
mo1 = 13;
}
jdint = 365.25*(date.y+yr1); /* truncates */
inter = 30.6001*(date.mo+mo1);
jdint = jdint+inter+date.d+jdzpt;
jd = jdint;
jdfrac=date.h/24.+date.mn/1440.+date.s/86400;
if(jdfrac < 0.5) {
jdint--;
jdfrac=jdfrac+0.5;
}
else jdfrac=jdfrac-0.5;
jd=jdint+jdfrac;
return(jd);
}
void caldat(jdin,date)
#define IGREG 2299161
double jdin;
struct date_time *date;
{
/* Returns date and time for a given julian date;
Adapted from Numerical Recipes, p. 12. */
int mm, id, iyyy; /* their notation */
long ja, jdint, jalpha, jb, jc, jd, je;
float jdfrac;
jdin = jdin + 0.5; /* adjust for 1/2 day */
jdint = jdin;
jdfrac = jdin - jdint;
date->h = jdfrac * 24; /* truncate */
date->mn = (jdfrac - ((float) date->h)/24.) * 1440.;
date->s = (jdfrac - ((float) date->h)/24. -
((float) date->mn)/1440.) * 86400;
if(jdint > IGREG) {
jalpha=((float) (jdint-1867216)-0.25)/36524.25;
ja=jdint+1+jalpha-(long)(0.25*jalpha);
}
else
ja=jdint;
jb=ja+1524;
jc=6680.0+((float) (jb-2439870)-122.1)/365.25;
jd=365*jc+(0.25*jc);
je=(jb-jd)/30.6001;
id=jb-jd-(int) (30.6001*je);
mm=je-1;
if(mm > 12) mm -= 12;
iyyy=jc-4715;
if(mm > 2) --iyyy;
if (iyyy <= 0) --iyyy;
date->y = iyyy;
date->mo = mm;
date->d = id;
}
void print_calendar(jdin,length)
double jdin;
short length;
{
struct date_time date;
char *months = "JanFebMarAprMayJunJulAugSepOctNovDec";
char mo_out[4];
caldat(jdin,&date);
mo_out[0] = *(months + 3*(date.mo - 1));
mo_out[1] = *(months + 3*(date.mo - 1) + 1);
mo_out[2] = *(months + 3*(date.mo - 1) + 2);
mo_out[3] = '\0';
if(length == 1)
printf("%d %s %d",date.y,mo_out,date.d);
else printf("%s %02d",mo_out,date.d); /*no year */
}
void print_time(jdin,prec)
double jdin;
short prec;
{
/* prints time only */
struct date_time date;
double temptime;
caldat(jdin,&date);
temptime = date.h + date.mn/60. + date.s/3600.;
put_coords(temptime,prec);
}
short day_of_week(jd)
double jd;
{
/* returns day of week, 0 = Mon, 6 = Sun. */
double x,y;
long i;
short d;
x = (jd+0.5)/7.;
d = 7.*(x - (long) x); /* truncate */
return(d);
}
void print_day(d)
short d;
{
char *days = "MonTueWedThuFriSatSun";
char day_out[4];
day_out[0] = *(days+3*d);
day_out[1] = *(days+3*d+1);
day_out[2] = *(days+3*d+2);
day_out[3] = '\0'; /* terminate with null char */
printf("%s",day_out);
}
double lst(jd,longit)
double jd,longit;
{
/* returns the local MEAN sidereal time (dec hrs) at julian date jd
at west longitude long (decimal hours). Follows
definitions in 1992 Astronomical Almanac, pp. B7 and L2.
Expression for GMST at 0h ut referenced to Aoki et al, A&A 105,
p.359, 1982. */
double t, ut, jdmid, jdint, jdfrac, sid_g, sid;
double jdnoon2000jan1 = 2451545.;
long jdin, sid_int;
jdin = jd; /* fossil code from earlier package which
split jd into integer and fractional parts ... */
jdint = jdin;
jdfrac = jd - jdint;
if(jdfrac < 0.5) {
jdmid = jdint - 0.5;
ut = jdfrac + 0.5;
}
else {
jdmid = jdint + 0.5;
ut = jdfrac - 0.5;
}
t = (jdmid - jdnoon2000jan1)/36525;
sid_g = (24110.54841+8640184.812866*t+0.093104*t*t-6.2e-6*t*t*t)/86400.;
sid_int = sid_g;
sid_g = sid_g - (double) sid_int;
sid_g = sid_g + 1.0027379093 * ut - longit/24.;
sid_int = sid_g;
sid_g = (sid_g - (double) sid_int) * 24.;
if(sid_g < 0.) sid_g = sid_g + 24.;
return(sid_g);
}
double adj_time(x)
double x;
{
/* adjusts a time (decimal hours) to be between -12 and 12. */
if(fabs(x) < 100000.) { /* too inefficient for this! */
while(x > 12.) {
x = x - 24.;
}
while(x < -12.) {
x = x + 24.;
}
}
else printf("Out of bounds in adj_time!\n");
return(x);
}
double circulo(x)
double x;
{
/* assuming x is an angle in degrees, returns
modulo 360 degrees. */
int n;
n = (int)(x / 360.);
return(x - 360. * n);
}
void geocent(geolong, geolat, height, x_geo, y_geo, z_geo)
double geolong, geolat, height, *x_geo, *y_geo, *z_geo;
/* computes the geocentric coordinates from the geodetic
(standard map-type) longitude, latitude, and height.
These are assumed to be in decimal hours, decimal degrees, and
meters respectively. Notation generally follows 1992 Astr Almanac,
p. K11 */
{
double denom, C_geo, S_geo;
geolat = geolat / DEG_IN_RADIAN;
geolong = geolong / HRS_IN_RADIAN;
denom = (1. - FLATTEN) * sin(geolat);
denom = cos(geolat) * cos(geolat) + denom*denom;
C_geo = 1. / sqrt(denom);
S_geo = (1. - FLATTEN) * (1. - FLATTEN) * C_geo;
C_geo = C_geo + height / EQUAT_RAD; /* deviation from almanac
notation -- include height here. */
S_geo = S_geo + height / EQUAT_RAD;
*x_geo = C_geo * cos(geolat) * cos(geolong);
*y_geo = C_geo * cos(geolat) * sin(geolong);
*z_geo = S_geo * sin(geolat);
}
void eclrot(jd, x, y, z)
/* rotates ecliptic rectangular coords x, y, z to
equatorial (all assumed of date.) */
double jd, *x, *y, *z;
{
double incl;
double xpr,ypr,zpr;
double T;
T = (jd - J2000) / 36525; /* centuries since J2000 */
incl = (23.439291 + T * (-0.0130042 - 0.00000016 * T))/DEG_IN_RADIAN;
/* 1992 Astron Almanac, p. B18, dropping the
cubic term, which is 2 milli-arcsec! */
ypr = cos(incl) * *y - sin(incl) * *z;
zpr = sin(incl) * *y + cos(incl) * *z;
*y = ypr;
*z = zpr;
/* x remains the same. */
}
double etcorr(jd)
double jd;
{
/* Given a julian date in 1900-2100, returns the jd corrected
for delta t; delta t is
TDT - UT (after 1983 and before 1994)
ET - UT (before 1983)
an extrapolated guess (after 1994).
For dates in the past (<= 1994 and after 1900) the value is linearly
interpolated on 5-year intervals; for dates after the present,
an extrapolation is used, because the true value of delta t
cannot be predicted precisely. Note that TDT is essentially the
modern version of ephemeris time with a slightly cleaner
definition.
Where the algorithm shifts there is an approximately 0.1 second
discontinuity. Also, the 5-year linear interpolation scheme can
lead to errors as large as 0.5 seconds in some cases, though
usually rather smaller. */
double jd1900 = 2415019.5;
double dates[20];
double delts[20]; /* can't initialize this look-up table
with stupid old sun compiler .... */
double year, delt;
int i;
/* this stupid patch for primitive sun C compilers ....
do not allow automatic initialization of arrays! */
for(i = 0; i <= 18; i++) dates[i] = 1900 + (double) i * 5.;
dates[19] = 1994;
delts[0] = -2.72; delts[1] = 3.86; delts[2] = 10.46;
delts[3] = 17.20; delts[4] = 21.16; delts[5] = 23.62;
delts[6] = 24.02; delts[7] = 23.93; delts[8] = 24.33;
delts[9] = 26.77; delts[10] = 29.15; delts[11] = 31.07;
delts[12] = 33.15; delts[13] = 35.73; delts[14] = 40.18;
delts[15] = 45.48; delts[16] = 50.54; delts[17] = 54.34;
delts[18] = 56.86; delts[19] = 59.98;
year = 1900. + (jd - 2415019.5) / 365.25;
if(year < 1994.0 && year >= 1900.) {
i = (year - 1900) / 5;
delt = delts[i] +
((delts[i+1] - delts[i])/(dates[i+1] - dates[i])) * (year - dates[i]);
}
else if (year > 1994. && year < 2100.)
delt = 33.15 + (2.164e-3) * (jd - 2436935.4); /* rough extrapolation */
else if (year < 1900) {
printf("etcorr ... no ephemeris time data for < 1900.\n");
delt = 0.;
}
else if (year >= 2100.) {
printf("etcorr .. very long extrapolation in delta T - inaccurate.\n");
delt = 180.; /* who knows? */
}
return(jd + delt/SEC_IN_DAY);
}
void accumoon(jd,geolat,lst,elevsea,topora,topodec,topodist)
double jd,geolat,lst,elevsea; /* jd, dec. degr., dec. hrs., meters */
double *topora,*topodec,*topodist;
/* More accurate (but more elaborate and slower) lunar
ephemeris, from Jean Meeus' *Astronomical Formulae For Calculators*,
pub. Willman-Bell. Includes all the terms given there. */
{
/* double *eclatit,*eclongit, *pie,*ra,*dec,*dist; geocent quantities,
formerly handed out but not in this version */
double pie, dist; /* horiz parallax */
double Lpr,M,Mpr,D,F,Om,T,Tsq,Tcb;
double e,lambda,B,beta,om1,om2;
double sinx, x, y, z, l, m, n;
double x_geo, y_geo, z_geo; /* geocentric position of *observer* */
jd = etcorr(jd); /* approximate correction to ephemeris time */
T = (jd - 2415020.) / 36525.; /* this based around 1900 ... */
Tsq = T * T;
Tcb = Tsq * T;
Lpr = 270.434164 + 481267.8831 * T - 0.001133 * Tsq
+ 0.0000019 * Tcb;
M = 358.475833 + 35999.0498*T - 0.000150*Tsq
- 0.0000033*Tcb;
Mpr = 296.104608 + 477198.8491*T + 0.009192*Tsq
+ 0.0000144*Tcb;
D = 350.737486 + 445267.1142*T - 0.001436 * Tsq
+ 0.0000019*Tcb;
F = 11.250889 + 483202.0251*T -0.003211 * Tsq
- 0.0000003*Tcb;
Om = 259.183275 - 1934.1420*T + 0.002078*Tsq
+ 0.0000022*Tcb;
Lpr = circulo(Lpr);
Mpr = circulo(Mpr);
M = circulo(M);
D = circulo(D);
F = circulo(F);
Om = circulo(Om);
sinx = sin((51.2 + 20.2 * T)/DEG_IN_RADIAN);
Lpr = Lpr + 0.000233 * sinx;
M = M - 0.001778 * sinx;
Mpr = Mpr + 0.000817 * sinx;
D = D + 0.002011 * sinx;
sinx = 0.003964 * sin((346.560+132.870*T -0.0091731*Tsq)/DEG_IN_RADIAN);
Lpr = Lpr + sinx;
Mpr = Mpr + sinx;
D = D + sinx;
F = F + sinx;
sinx = sin(Om/DEG_IN_RADIAN);
Lpr = Lpr + 0.001964 * sinx;
Mpr = Mpr + 0.002541 * sinx;
D = D + 0.001964 * sinx;
F = F - 0.024691 * sinx;
F = F - 0.004328 * sin((Om + 275.05 -2.30*T)/DEG_IN_RADIAN);
e = 1 - 0.002495 * T - 0.00000752 * Tsq;
M = M / DEG_IN_RADIAN; /* these will all be arguments ... */
Mpr = Mpr / DEG_IN_RADIAN;
D = D / DEG_IN_RADIAN;
F = F / DEG_IN_RADIAN;
lambda = Lpr + 6.288750 * sin(Mpr)
+ 1.274018 * sin(2*D - Mpr)
+ 0.658309 * sin(2*D)
+ 0.213616 * sin(2*Mpr)
- e * 0.185596 * sin(M)
- 0.114336 * sin(2*F)
+ 0.058793 * sin(2*D - 2*Mpr)
+ e * 0.057212 * sin(2*D - M - Mpr)
+ 0.053320 * sin(2*D + Mpr)
+ e * 0.045874 * sin(2*D - M)
+ e * 0.041024 * sin(Mpr - M)
- 0.034718 * sin(D)
- e * 0.030465 * sin(M+Mpr)
+ 0.015326 * sin(2*D - 2*F)
- 0.012528 * sin(2*F + Mpr)
- 0.010980 * sin(2*F - Mpr)
+ 0.010674 * sin(4*D - Mpr)
+ 0.010034 * sin(3*Mpr)
+ 0.008548 * sin(4*D - 2*Mpr)
- e * 0.007910 * sin(M - Mpr + 2*D)
- e * 0.006783 * sin(2*D + M)
+ 0.005162 * sin(Mpr - D);
/* And furthermore.....*/
lambda = lambda + e * 0.005000 * sin(M + D)
+ e * 0.004049 * sin(Mpr - M + 2*D)
+ 0.003996 * sin(2*Mpr + 2*D)
+ 0.003862 * sin(4*D)
+ 0.003665 * sin(2*D - 3*Mpr)
+ e * 0.002695 * sin(2*Mpr - M)
+ 0.002602 * sin(Mpr - 2*F - 2*D)
+ e * 0.002396 * sin(2*D - M - 2*Mpr)
- 0.002349 * sin(Mpr + D)
+ e * e * 0.002249 * sin(2*D - 2*M)
- e * 0.002125 * sin(2*Mpr + M)
- e * e * 0.002079 * sin(2*M)
+ e * e * 0.002059 * sin(2*D - Mpr - 2*M)
- 0.001773 * sin(Mpr + 2*D - 2*F)
- 0.001595 * sin(2*F + 2*D)
+ e * 0.001220 * sin(4*D - M - Mpr)
- 0.001110 * sin(2*Mpr + 2*F)
+ 0.000892 * sin(Mpr - 3*D)
- e * 0.000811 * sin(M + Mpr + 2*D)
+ e * 0.000761 * sin(4*D - M - 2*Mpr)
+ e * e * 0.000717 * sin(Mpr - 2*M)
+ e * e * 0.000704 * sin(Mpr - 2 * M - 2*D)
+ e * 0.000693 * sin(M - 2*Mpr + 2*D)
+ e * 0.000598 * sin(2*D - M - 2*F)
+ 0.000550 * sin(Mpr + 4*D)
+ 0.000538 * sin(4*Mpr)
+ e * 0.000521 * sin(4*D - M)
+ 0.000486 * sin(2*Mpr - D);
/* *eclongit = lambda; */
B = 5.128189 * sin(F)
+ 0.280606 * sin(Mpr + F)
+ 0.277693 * sin(Mpr - F)
+ 0.173238 * sin(2*D - F)
+ 0.055413 * sin(2*D + F - Mpr)
+ 0.046272 * sin(2*D - F - Mpr)
+ 0.032573 * sin(2*D + F)
+ 0.017198 * sin(2*Mpr + F)
+ 0.009267 * sin(2*D + Mpr - F)
+ 0.008823 * sin(2*Mpr - F)
+ e * 0.008247 * sin(2*D - M - F)
+ 0.004323 * sin(2*D - F - 2*Mpr)
+ 0.004200 * sin(2*D + F + Mpr)
+ e * 0.003372 * sin(F - M - 2*D)
+ 0.002472 * sin(2*D + F - M - Mpr)
+ e * 0.002222 * sin(2*D + F - M)
+ e * 0.002072 * sin(2*D - F - M - Mpr)
+ e * 0.001877 * sin(F - M + Mpr)
+ 0.001828 * sin(4*D - F - Mpr)
- e * 0.001803 * sin(F + M)
- 0.001750 * sin(3*F)
+ e * 0.001570 * sin(Mpr - M - F)
- 0.001487 * sin(F + D)
- e * 0.001481 * sin(F + M + Mpr)
+ e * 0.001417 * sin(F - M - Mpr)
+ e * 0.001350 * sin(F - M)
+ 0.001330 * sin(F - D)
+ 0.001106 * sin(F + 3*Mpr)
+ 0.001020 * sin(4*D - F)
+ 0.000833 * sin(F + 4*D - Mpr);
/* not only that, but */
B = B + 0.000781 * sin(Mpr - 3*F)
+ 0.000670 * sin(F + 4*D - 2*Mpr)
+ 0.000606 * sin(2*D - 3*F)
+ 0.000597 * sin(2*D + 2*Mpr - F)
+ e * 0.000492 * sin(2*D + Mpr - M - F)
+ 0.000450 * sin(2*Mpr - F - 2*D)
+ 0.000439 * sin(3*Mpr - F)
+ 0.000423 * sin(F + 2*D + 2*Mpr)
+ 0.000422 * sin(2*D - F - 3*Mpr)
- e * 0.000367 * sin(M + F + 2*D - Mpr)
- e * 0.000353 * sin(M + F + 2*D)
+ 0.000331 * sin(F + 4*D)
+ e * 0.000317 * sin(2*D + F - M + Mpr)
+ e * e * 0.000306 * sin(2*D - 2*M - F)
- 0.000283 * sin(Mpr + 3*F);
om1 = 0.0004664 * cos(Om/DEG_IN_RADIAN);
om2 = 0.0000754 * cos((Om + 275.05 - 2.30*T)/DEG_IN_RADIAN);
beta = B * (1. - om1 - om2);
/* *eclatit = beta; */
pie = 0.950724
+ 0.051818 * cos(Mpr)
+ 0.009531 * cos(2*D - Mpr)
+ 0.007843 * cos(2*D)
+ 0.002824 * cos(2*Mpr)
+ 0.000857 * cos(2*D + Mpr)
+ e * 0.000533 * cos(2*D - M)
+ e * 0.000401 * cos(2*D - M - Mpr)
+ e * 0.000320 * cos(Mpr - M)
- 0.000271 * cos(D)
- e * 0.000264 * cos(M + Mpr)
- 0.000198 * cos(2*F - Mpr)
+ 0.000173 * cos(3*Mpr)
+ 0.000167 * cos(4*D - Mpr)
- e * 0.000111 * cos(M)
+ 0.000103 * cos(4*D - 2*Mpr)
- 0.000084 * cos(2*Mpr - 2*D)
- e * 0.000083 * cos(2*D + M)
+ 0.000079 * cos(2*D + 2*Mpr)
+ 0.000072 * cos(4*D)
+ e * 0.000064 * cos(2*D - M + Mpr)
- e * 0.000063 * cos(2*D + M - Mpr)
+ e * 0.000041 * cos(M + D)
+ e * 0.000035 * cos(2*Mpr - M)
- 0.000033 * cos(3*Mpr - 2*D)
- 0.000030 * cos(Mpr + D)
- 0.000029 * cos(2*F - 2*D)
- e * 0.000029 * cos(2*Mpr + M)
+ e * e * 0.000026 * cos(2*D - 2*M)
- 0.000023 * cos(2*F - 2*D + Mpr)
+ e * 0.000019 * cos(4*D - M - Mpr);
beta = beta/DEG_IN_RADIAN;
lambda = lambda/DEG_IN_RADIAN;
l = cos(lambda) * cos(beta);
m = sin(lambda) * cos(beta);
n = sin(beta);
eclrot(jd,&l,&m,&n);
dist = 1/sin((pie)/DEG_IN_RADIAN);
x = l * dist;
y = m * dist;
z = n * dist;
/* *ra = atan_circ(l,m) * DEG_IN_RADIAN;
*dec = asin(n) * DEG_IN_RADIAN; */
geocent(lst,geolat,elevsea,&x_geo,&y_geo,&z_geo);
x = x - x_geo; /* topocentric correction using elliptical earth fig. */
y = y - y_geo;
z = z - z_geo;
*topodist = sqrt(x*x + y*y + z*z);
l = x / (*topodist);
m = y / (*topodist);
n = z / (*topodist);
*topora = atan_circ(l,m) * HRS_IN_RADIAN;
*topodec = asin(n) * DEG_IN_RADIAN;
}
lpsun(jd,ra,dec)
double jd, *ra, *dec;
/* Low precision formulae for the sun, from Almanac p. C24 (1990) */
/* ra and dec are returned as decimal hours and decimal degrees. */
{
double n, L, g, lambda,epsilon,alpha,delta,x,y,z;
n = jd - 2451545.0;
L = 280.460 + 0.9856474 * n;
g = (357.528 + 0.9856003 * n)/DEG_IN_RADIAN;
lambda = (L + 1.915 * sin(g) + 0.020 * sin(2. * g))/DEG_IN_RADIAN;
epsilon = (23.439 - 0.0000004 * n)/DEG_IN_RADIAN;
x = cos(lambda);
y = cos(epsilon) * sin(lambda);
z = sin(epsilon)*sin(lambda);
*ra = (atan_circ(x,y))*HRS_IN_RADIAN;
*dec = (asin(z))*DEG_IN_RADIAN;
}
double jd_moon_alt(alt,jdguess,lat,longit)
double alt, jdguess, lat, longit;
{
/* returns jd at which moon is at a given
altitude, given jdguess as a starting point. */
double jdout;
double deriv, err, del = 0.002;
double ra,dec,dist,sid,ha,alt2,alt3;
short i = 0;
/* first guess */
sid=lst(jdguess,longit);
accumoon(jdguess,lat,sid,0.,&ra,&dec,&dist);
ha = lst(jdguess,longit) - ra;
alt2 = altit(dec,ha,lat);
jdguess = jdguess + del;
sid = lst(jdguess,longit);
accumoon(jdguess,lat,sid,0.,&ra,&dec,&dist);
alt3 = altit(dec,(sid - ra),lat);
err = alt3 - alt;
deriv = (alt3 - alt2) / del;
while((fabs(err) > 0.01) && (i < 10)) {
jdguess = jdguess - err/deriv;
sid=lst(jdguess,longit);
accumoon(jdguess,lat,sid,0.,&ra,&dec,&dist);
alt3 = altit(dec,(sid - ra),lat);
err = alt3 - alt;
i++;
if(i == 9) return (-1.0e10); /* bad status flag */
}
jdout = jdguess;
return(jdout);
}