dockapps/wmmoonclock/src/MoonRise.c
2014-10-05 19:18:49 +01:00

174 lines
3.5 KiB
C

#include <stdio.h>
#include <math.h>
#include "MoonRise.h"
#include "Moon.h"
#define DegPerRad 57.29577951308232087680
#define RadPerDeg 0.01745329251994329576
extern double Glon, SinGlat, CosGlat, TimeZone;
void MoonRise(int year, int month, int day, double LocalHour, double *UTRise, double *UTSet){
double UT, ym, y0, yp, SinH0;
double xe, ye, z1, z2, SinH(), hour24();
int Rise, Set, nz;
SinH0 = sin( 8.0/60.0 * RadPerDeg );
UT = 1.0+TimeZone;
*UTRise = -999.0;
*UTSet = -999.0;
Rise = Set = 0;
ym = SinH(year, month, day, UT-1.0) - SinH0;
while ( (UT <= 24.0+TimeZone) ) {
y0 = SinH(year, month, day, UT) - SinH0;
yp = SinH(year, month, day, UT+1.0) - SinH0;
Interp(ym, y0, yp, &xe, &ye, &z1, &z2, &nz);
switch(nz){
case 0:
break;
case 1:
if (ym < 0.0){
*UTRise = UT + z1;
Rise = 1;
} else {
*UTSet = UT + z1;
Set = 1;
}
break;
case 2:
if (ye < 0.0){
*UTRise = UT + z2;
*UTSet = UT + z1;
} else {
*UTRise = UT + z1;
*UTSet = UT + z2;
}
Rise = 1;
Set = 1;
break;
}
ym = yp;
UT += 2.0;
}
if (Rise){
*UTRise -= TimeZone;
*UTRise = hour24(*UTRise);
} else {
*UTRise = -999.0;
}
if (Set){
*UTSet -= TimeZone;
*UTSet = hour24(*UTSet);
} else {
*UTSet = -999.0;
}
}
void UTTohhmm(double UT, int *h, int *m){
if (UT < 0.0) {
*h = -1.0;
*m = -1.0;
} else {
*h = (int)UT;
*m = (int)((UT-(double)(*h))*60.0+0.5);
if (*m == 60) {
/*
* If it was 23:60 this should become 24:00
* I prefer this designation to 00:00. So dont reset h to 0 when it goes above 24.
*/
*h += 1;
*m = 0;
}
}
}
void Interp(double ym, double y0, double yp, double *xe, double *ye, double *z1, double *z2, int *nz){
double a, b, c, d, dx;
*nz = 0;
a = 0.5*(ym+yp)-y0;
b = 0.5*(yp-ym);
c = y0;
*xe = -b/(2.0*a);
*ye = (a*(*xe) + b) * (*xe) + c;
d = b*b - 4.0*a*c;
if (d >= 0){
dx = 0.5*sqrt(d)/fabs(a);
*z1 = *xe - dx;
*z2 = *xe+dx;
if (fabs(*z1) <= 1.0) *nz += 1;
if (fabs(*z2) <= 1.0) *nz += 1;
if (*z1 < -1.0) *z1 = *z2;
}
}
double SinH(int year, int month, int day, double UT){
double TU, frac(), jd();
double RA_Moon, DEC_Moon, gmst, lmst, Tau, Moon();
double angle2pi();
TU = (jd(year, month, day, UT) - 2451545.0)/36525.0;
/* this is more accurate, but wasteful for this -- use low res approx.
TU2 = TU*TU;
TU3 = TU2*TU;
Moon(TU, &LambdaMoon, &BetaMoon, &R, &AGE);
LambdaMoon *= RadPerDeg;
BetaMoon *= RadPerDeg;
epsilon = (23.43929167 - 0.013004166*TU - 1.6666667e-7*TU2 - 5.0277777778e-7*TU3)*RadPerDeg;
RA_Moon = angle2pi(atan2(sin(LambdaMoon)*cos(epsilon)-tan(BetaMoon)*sin(epsilon), cos(LambdaMoon)));
DEC_Moon = asin( sin(BetaMoon)*cos(epsilon) + cos(BetaMoon)*sin(epsilon)*sin(LambdaMoon));
*/
MiniMoon(TU, &RA_Moon, &DEC_Moon);
RA_Moon *= 15.0*RadPerDeg;
DEC_Moon *= RadPerDeg;
/*
* Compute Greenwich Mean Sidereal Time (gmst)
*/
UT = 24.0*frac( UT/24.0 );
/* this is for the ephemeris meridian???
gmst = 6.697374558 + 1.0027379093*UT + (8640184.812866+(0.093104-6.2e-6*TU)*TU)*TU/3600.0;
*/
gmst = UT + 6.697374558 + (8640184.812866+(0.093104-6.2e-6*TU)*TU)*TU/3600.0;
lmst = 24.0*frac( (gmst-Glon/15.0) / 24.0 );
Tau = 15.0*lmst*RadPerDeg - RA_Moon;
return( SinGlat*sin(DEC_Moon) + CosGlat*cos(DEC_Moon)*cos(Tau) );
}