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	git-svn-id: svn+ssh://svn.code.sf.net/p/wsjt/wsjt/branches/wsjtx@3839 ab8295b8-cf94-4d9e-aec4-7959e3be5d79
		
			
				
	
	
		
			89 lines
		
	
	
		
			2.8 KiB
		
	
	
	
		
			Fortran
		
	
	
	
	
	
			
		
		
	
	
			89 lines
		
	
	
		
			2.8 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                           !UT!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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