400 lines
9.1 KiB
C
400 lines
9.1 KiB
C
#include "CalcEphem.h"
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#include <math.h>
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#include <string.h>
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void CalcEphem(date, UT, c)
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long int date; /* integer containing the date (e.g. 960829) */
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double UT; /* Universal Time */
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CTrans *c; /* structure containing all the relevent coord trans info */
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{
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int year, month, day;
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double TU, TU2, TU3, T0;
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double varep, varpi;
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double eccen, epsilon;
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double days, M, E, nu, lambnew;
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double r0, earth_sun_distance;
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double RA, DEC, RA_Moon, DEC_Moon;
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double TDT, AGE, LambdaMoon, BetaMoon, R;
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double jd(), hour24(), angle2pi(), angle360(), kepler(), Moon(), NewMoon();
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double Ta, Tb, Tc, frac();
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double SinGlat, CosGlat, Tau, lmst, x, y, z;
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double SinTau, CosTau, SinDec, CosDec;
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c->UT = UT;
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year = (int)(date/10000);
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month = (int)( (date - year*10000)/100 );
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day = (int)( date - year*10000 - month*100 );
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c->year = year;
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c->month = month;
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c->day = day;
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c->doy = DayofYear(year, month, day);
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c->dow = DayofWeek(year, month, day, c->dowstr);
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/*
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* Compute Greenwich Mean Sidereal Time (gmst)
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* The TU here is number of Julian centuries
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* since 2000 January 1.5
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* From the 1996 astronomical almanac
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*/
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TU = (jd(year, month, day, 0.0) - 2451545.0)/36525.0;
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TU2 = TU*TU;
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TU3 = TU2*TU;
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T0 = (6.0 + 41.0/60.0 + 50.54841/3600.0) + 8640184.812866/3600.0*TU
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+ 0.093104/3600.0*TU2 - 6.2e-6/3600.0*TU3;
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T0 = hour24(T0);
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c->gmst = hour24(T0 + UT*1.002737909);
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lmst = 24.0*frac( (c->gmst - c->Glon/15.0) / 24.0 );
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/*
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*
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* Construct Transformation Matrix from GEI to GSE systems
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*
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*
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* First compute:
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* mean ecliptic longitude of sun at epoch TU (varep)
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* elciptic longitude of perigee at epoch TU (varpi)
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* eccentricity of orbit at epoch TU (eccen)
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*
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* The TU here is the number of Julian centuries since
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* 1900 January 0.0 (= 2415020.0)
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*/
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TDT = UT + 59.0/3600.0;
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TU = (jd(year, month, day, TDT) - 2415020.0)/36525.0;
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varep = (279.6966778 + 36000.76892*TU + 0.0003025*TU*TU)*RadPerDeg;
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varpi = (281.2208444 + 1.719175*TU + 0.000452778*TU*TU)*RadPerDeg;
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eccen = 0.01675104 - 0.0000418*TU - 0.000000126*TU*TU;
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c->eccentricity = eccen;
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/*
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* Compute the Obliquity of the Ecliptic at epoch TU
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* The TU in this formula is the number of Julian
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* centuries since epoch 2000 January 1.5
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*/
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TU = (jd(year, month, day, TDT) - jd(2000, 1, 1, 12.0))/36525.0;
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epsilon = (23.43929167 - 0.013004166*TU - 1.6666667e-7*TU*TU
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- 5.0277777778e-7*TU*TU*TU)*RadPerDeg;
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c->epsilon = epsilon;
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/*
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* Compute:
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* Number of Days since epoch 1990.0 (days)
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* The Mean Anomaly (M)
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* The True Anomaly (nu)
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* The Eccentric Anomaly via Keplers equation (E)
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*
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*
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*/
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days = jd(year, month, day, TDT) - jd(year, month, day, TDT);
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M = angle2pi(2.0*M_PI/365.242191*days + varep - varpi);
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E = kepler(M, eccen);
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nu = 2.0*atan( sqrt((1.0+eccen)/(1.0-eccen))*tan(E/2.0) );
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lambnew = angle2pi(nu + varpi);
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c->lambda_sun = lambnew;
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/*
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* Compute distance from earth to the sun
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*/
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r0 = 1.495985e8; /* in km */
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earth_sun_distance = r0*(1-eccen*eccen)/(1.0 + eccen*cos(nu))/6371.2;
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c->earth_sun_dist = earth_sun_distance;
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/*
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* Compute Right Ascension and Declination of the Sun
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*/
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RA = angle360(atan2(sin(lambnew)*cos(epsilon), cos(lambnew))*180.0/M_PI);
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DEC = asin(sin(epsilon)*sin(lambnew))*180.0/M_PI;
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c->RA_sun = RA;
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c->DEC_sun = DEC;
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/*
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* Compute Moon Phase and AGE Stuff. The AGE that comes out of Moon()
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* is actually the Phase converted to days. Since AGE is actually defined
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* to be time since last NewMoon, we need to figure out what the JD of the
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* last new moon was. Thats done below....
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*/
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TU = (jd(year, month, day, TDT) - 2451545.0)/36525.0;
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c->MoonPhase = Moon(TU, &LambdaMoon, &BetaMoon, &R, &AGE);
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LambdaMoon *= RadPerDeg;
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BetaMoon *= RadPerDeg;
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RA_Moon = angle360(atan2(sin(LambdaMoon)*cos(epsilon)-tan(BetaMoon)*sin(epsilon), cos(LambdaMoon))*DegPerRad);
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DEC_Moon = asin( sin(BetaMoon)*cos(epsilon) + cos(BetaMoon)*sin(epsilon)*sin(LambdaMoon))*DegPerRad;
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c->RA_moon = RA_Moon;
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c->DEC_moon = DEC_Moon;
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/*
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* Compute Alt/Az coords
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*/
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Tau = (15.0*lmst - RA_Moon)*RadPerDeg;
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CosGlat = cos(c->Glat*RadPerDeg); SinGlat = sin(c->Glat*RadPerDeg);
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CosTau = cos(Tau); SinTau = sin(Tau);
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SinDec = sin(DEC_Moon*RadPerDeg); CosDec = cos(DEC_Moon*RadPerDeg);
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x = CosDec*CosTau*SinGlat - SinDec*CosGlat;
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y = CosDec*SinTau;
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z = CosDec*CosTau*CosGlat + SinDec*SinGlat;
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c->A_moon = DegPerRad*atan2(y, x);
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c->h_moon = DegPerRad*asin(z);
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c->Visible = (c->h_moon < 0.0) ? 0 : 1;
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/*
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* Compute accurate AGE of the Moon
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*/
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Tb = TU - AGE/36525.0; /* should be very close to minimum */
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Ta = Tb - 0.4/36525.0;
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Tc = Tb + 0.4/36525.0;
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c->MoonAge = (TU - NewMoon(Ta, Tb, Tc))*36525.0;
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/*
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* Compute Earth-Moon distance
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*/
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c->EarthMoonDistance = R;
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}
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double kepler(M, e)
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double M, e;
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{
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int n=0;
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double E, Eold, eps = 1.0e-8;
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E = M + e*sin(M);
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do{
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Eold = E;
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E = Eold + (M-Eold+e*sin(Eold))
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/(1.0-e*cos(Eold));
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++n;
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}while((fabs(E-Eold) > eps) && (n < 100));
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return(E);
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}
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int DayofYear(year, month, day)
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int year, month, day;
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{
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double jd();
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return((int)(jd(year, month, day, 0.0) - jd(year, 1, 0, 0.0)));
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}
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int DayofWeek(year, month, day, dowstr)
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int year, month, day;
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char dowstr[];
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{
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double JD, A, Afrac, jd();
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int n, iA;
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JD = jd(year, month, day, 0.0);
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A = (JD + 1.5)/7.0;
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iA = (int)A;
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Afrac = A - (double)iA;
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n = (int)(Afrac*7.0 + 0.5);
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switch(n){
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case 0:
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strcpy(dowstr, "Sunday");
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break;
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case 1:
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strcpy(dowstr, "Monday");
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break;
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case 2:
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strcpy(dowstr, "Tuesday");
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break;
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case 3:
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strcpy(dowstr, "Wednesday");
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break;
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case 4:
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strcpy(dowstr, "Thursday");
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break;
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case 5:
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strcpy(dowstr, "Friday");
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break;
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case 6:
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strcpy(dowstr, "Saturday");
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break;
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}
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return(n);
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}
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/*
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* Compute the Julian Day number for the given date.
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* Julian Date is the number of days since noon of Jan 1 4713 B.C.
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*/
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double jd(ny, nm, nd, UT)
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int ny, nm, nd;
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double UT;
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{
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double A, B, C, D, JD, day;
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day = nd + UT/24.0;
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if ((nm == 1) || (nm == 2)){
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ny = ny - 1;
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nm = nm + 12;
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}
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if (((double)ny+nm/12.0+day/365.25)>=(1582.0+10.0/12.0+15.0/365.25)){
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A = ((int)(ny / 100.0));
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B = 2.0 - A + (int)(A/4.0);
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}
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else{
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B = 0.0;
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}
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if (ny < 0.0){
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C = (int)((365.25*(double)ny) - 0.75);
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}
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else{
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C = (int)(365.25*(double)ny);
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}
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D = (int)(30.6001*(double)(nm+1));
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JD = B + C + D + day + 1720994.5;
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return(JD);
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}
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double hour24(hour)
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double hour;
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{
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int n;
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if (hour < 0.0){
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n = (int)(hour/24.0) - 1;
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return(hour-n*24.0);
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}
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else if (hour > 24.0){
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n = (int)(hour/24.0);
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return(hour-n*24.0);
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}
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else{
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return(hour);
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}
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}
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double angle2pi(angle)
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double angle;
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{
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int n;
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double a;
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a = 2.0*M_PI;
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if (angle < 0.0){
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n = (int)(angle/a) - 1;
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return(angle-n*a);
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}
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else if (angle > a){
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n = (int)(angle/a);
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return(angle-n*a);
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}
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else{
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return(angle);
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}
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}
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double angle360(angle)
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double angle;
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{
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int n;
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if (angle < 0.0){
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n = (int)(angle/360.0) - 1;
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return(angle-n*360.0);
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}
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else if (angle > 360.0){
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n = (int)(angle/360.0);
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return(angle-n*360.0);
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}
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else{
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return(angle);
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}
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}
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void Radec_to_Cart(ra, dec, r)
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double ra, dec; /* RA and DEC */
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Vector *r; /* returns corresponding cartesian unit vector */
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{
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/*
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* Convert ra/dec from degrees to radians
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*/
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ra *= RadPerDeg;
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dec *= RadPerDeg;
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/*
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* Compute cartesian coordinates (in GEI)
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*/
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r->x = cos(dec) * cos(ra);
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r->y = cos(dec) * sin(ra);
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r->z = sin(dec);
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}
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int LeapYear(year)
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int year;
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{
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if ((year%100 == 0)&&(year%400 != 0)) return(0);
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else if (year%4 == 0) return(1);
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else return(0);
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}
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