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authorJoseph Hunkeler <jhunkeler@gmail.com>2015-07-08 20:46:52 -0400
committerJoseph Hunkeler <jhunkeler@gmail.com>2015-07-08 20:46:52 -0400
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+.help pa Jun99 "Slalib Package"
+.nf
+
+ DOUBLE PRECISION FUNCTION slPA (HA, DEC, PHI)
+
+ - - -
+ P A
+ - - -
+
+ HA, Dec to Parallactic Angle (double precision)
+
+ Given:
+ HA d hour angle in radians (geocentric apparent)
+ DEC d declination in radians (geocentric apparent)
+ PHI d observatory latitude in radians (geodetic)
+
+ The result is in the range -pi to +pi
+
+ Notes:
+
+ 1) The parallactic angle at a point in the sky is the position
+ angle of the vertical, i.e. the angle between the direction to
+ the pole and to the zenith. In precise applications care must
+ be taken only to use geocentric apparent HA,Dec and to consider
+ separately the effects of atmospheric refraction and telescope
+ mount errors.
+
+ 2) At the pole a zero result is returned.
+
+ P.T.Wallace Starlink 16 August 1994
+
+ Copyright (C) 1995 Rutherford Appleton Laboratory
+ Copyright (C) 1995 Association of Universities for Research in Astronomy Inc.
+
+.fi
+.endhelp