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authorJoseph Hunkeler <jhunkeler@gmail.com>2015-03-04 21:21:30 -0500
committerJoseph Hunkeler <jhunkeler@gmail.com>2015-03-04 21:21:30 -0500
commitd54fe7c1f704a63824c5bfa0ece65245572e9b27 (patch)
treeafc52015ffc2c74e0266653eecef1c8ef8ba5d91 /src/slalib/de2h.f
downloadcalfuse-d54fe7c1f704a63824c5bfa0ece65245572e9b27.tar.gz
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+ SUBROUTINE sla_DE2H (HA, DEC, PHI, AZ, EL)
+*+
+* - - - - -
+* D E 2 H
+* - - - - -
+*
+* Equatorial to horizon coordinates: HA,Dec to Az,El
+*
+* (double precision)
+*
+* Given:
+* HA d hour angle
+* DEC d declination
+* PHI d observatory latitude
+*
+* Returned:
+* AZ d azimuth
+* EL d elevation
+*
+* Notes:
+*
+* 1) All the arguments are angles in radians.
+*
+* 2) Azimuth is returned in the range 0-2pi; north is zero,
+* and east is +pi/2. Elevation is returned in the range
+* +/-pi/2.
+*
+* 3) The latitude must be geodetic. In critical applications,
+* corrections for polar motion should be applied.
+*
+* 4) In some applications it will be important to specify the
+* correct type of hour angle and declination in order to
+* produce the required type of azimuth and elevation. In
+* particular, it may be important to distinguish between
+* elevation as affected by refraction, which would
+* require the "observed" HA,Dec, and the elevation
+* in vacuo, which would require the "topocentric" HA,Dec.
+* If the effects of diurnal aberration can be neglected, the
+* "apparent" HA,Dec may be used instead of the topocentric
+* HA,Dec.
+*
+* 5) No range checking of arguments is carried out.
+*
+* 6) In applications which involve many such calculations, rather
+* than calling the present routine it will be more efficient to
+* use inline code, having previously computed fixed terms such
+* as sine and cosine of latitude, and (for tracking a star)
+* sine and cosine of declination.
+*
+* P.T.Wallace Starlink 9 July 1994
+*
+* Copyright (C) 1995 Rutherford Appleton Laboratory
+*-
+
+ IMPLICIT NONE
+
+ DOUBLE PRECISION HA,DEC,PHI,AZ,EL
+
+ DOUBLE PRECISION D2PI
+ PARAMETER (D2PI=6.283185307179586476925286766559D0)
+
+ DOUBLE PRECISION SH,CH,SD,CD,SP,CP,X,Y,Z,R,A
+
+
+* Useful trig functions
+ SH=SIN(HA)
+ CH=COS(HA)
+ SD=SIN(DEC)
+ CD=COS(DEC)
+ SP=SIN(PHI)
+ CP=COS(PHI)
+
+* Az,El as x,y,z
+ X=-CH*CD*SP+SD*CP
+ Y=-SH*CD
+ Z=CH*CD*CP+SD*SP
+
+* To spherical
+ R=SQRT(X*X+Y*Y)
+ IF (R.EQ.0D0) THEN
+ A=0D0
+ ELSE
+ A=ATAN2(Y,X)
+ END IF
+ IF (A.LT.0D0) A=A+D2PI
+ AZ=A
+ EL=ATAN2(Z,R)
+
+ END