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89 lines
2.7 KiB
Fortran
89 lines
2.7 KiB
Fortran
subroutine sun(y,m,DD,UT,lon,lat,RA,Dec,LST,Az,El,mjd,day)
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implicit none
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integer y !Year
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integer m !Month
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integer DD !Day
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integer mjd !Modified Julian Date
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real UT !UTC in hours
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real RA,Dec !RA and Dec of sun
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! NB: Double caps here are single caps in the writeup.
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! Orbital elements of the Sun (also N=0, i=0, a=1):
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real w !Argument of perihelion
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real e !Eccentricity
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real MM !Mean anomaly
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real Ls !Mean longitude
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! Other standard variables:
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real v !True anomaly
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real EE !Eccentric anomaly
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real ecl !Obliquity of the ecliptic
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real d !Ephemeris time argument in days
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real r !Distance to sun, AU
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real xv,yv !x and y coords in ecliptic
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real lonsun !Ecliptic long and lat of sun
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! Ecliptic coords of sun (geocentric)
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real xs,ys
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! Equatorial coords of sun (geocentric)
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real xe,ye,ze
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real lon,lat
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real GMST0,LST,HA
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real xx,yy,zz
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real xhor,yhor,zhor
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real Az,El
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real day
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real rad
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data rad/57.2957795/
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! Time in days, with Jan 0, 2000 equal to 0.0:
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d=367*y - 7*(y+(m+9)/12)/4 + 275*m/9 + DD - 730530 + UT/24.0
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mjd=d + 51543
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ecl = 23.4393 - 3.563e-7 * d
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! Compute updated orbital elements for Sun:
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w = 282.9404 + 4.70935e-5 * d
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e = 0.016709 - 1.151e-9 * d
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MM = mod(356.0470d0 + 0.9856002585d0 * d + 360000.d0,360.d0)
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Ls = mod(w+MM+720.0,360.0)
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EE = MM + e*rad*sin(MM/rad) * (1.0 + e*cos(M/rad))
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EE = EE - (EE - e*rad*sin(EE/rad)-MM) / (1.0 - e*cos(EE/rad))
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xv = cos(EE/rad) - e
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yv = sqrt(1.0-e*e) * sin(EE/rad)
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v = rad*atan2(yv,xv)
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r = sqrt(xv*xv + yv*yv)
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lonsun = mod(v + w + 720.0,360.0)
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! Ecliptic coordinates of sun (rectangular):
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xs = r * cos(lonsun/rad)
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ys = r * sin(lonsun/rad)
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! Equatorial coordinates of sun (rectangular):
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xe = xs
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ye = ys * cos(ecl/rad)
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ze = ys * sin(ecl/rad)
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! RA and Dec in degrees:
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RA = rad*atan2(ye,xe)
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Dec = rad*atan2(ze,sqrt(xe*xe + ye*ye))
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GMST0 = (Ls + 180.0)/15.0
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LST = mod(GMST0+UT+lon/15.0+48.0,24.0) !LST in hours
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HA = 15.0*LST - RA !HA in degrees
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xx = cos(HA/rad)*cos(Dec/rad)
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yy = sin(HA/rad)*cos(Dec/rad)
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zz = sin(Dec/rad)
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xhor = xx*sin(lat/rad) - zz*cos(lat/rad)
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yhor = yy
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zhor = xx*cos(lat/rad) + zz*sin(lat/rad)
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Az = mod(rad*atan2(yhor,xhor) + 180.0 + 360.0,360.0)
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El = rad*asin(zhor)
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day=d-1.5
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return
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end subroutine sun
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