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author | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
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committer | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
commit | 40e5a5811c6ffce9b0974e93cdd927cbcf60c157 (patch) | |
tree | 4464880c571602d54f6ae114729bf62a89518057 /math/slalib/pa.f | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'math/slalib/pa.f')
-rw-r--r-- | math/slalib/pa.f | 64 |
1 files changed, 64 insertions, 0 deletions
diff --git a/math/slalib/pa.f b/math/slalib/pa.f new file mode 100644 index 00000000..88d21105 --- /dev/null +++ b/math/slalib/pa.f @@ -0,0 +1,64 @@ + 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 +* +* License: +* This program is free software; you can redistribute it and/or modify +* it under the terms of the GNU General Public License as published by +* the Free Software Foundation; either version 2 of the License, or +* (at your option) any later version. +* +* This program is distributed in the hope that it will be useful, +* but WITHOUT ANY WARRANTY; without even the implied warranty of +* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the +* GNU General Public License for more details. +* +* You should have received a copy of the GNU General Public License +* along with this program (see SLA_CONDITIONS); if not, write to the +* Free Software Foundation, Inc., 51 Franklin Street, Fifth Floor, +* Boston, MA 02110-1301 USA +* +* Copyright (C) 1995 Association of Universities for Research in Astronomy Inc. +*- + + IMPLICIT NONE + + DOUBLE PRECISION HA,DEC,PHI + + DOUBLE PRECISION CP,SQSZ,CQSZ + + + + CP=COS(PHI) + SQSZ=CP*SIN(HA) + CQSZ=SIN(PHI)*COS(DEC)-CP*SIN(DEC)*COS(HA) + IF (SQSZ.EQ.0D0.AND.CQSZ.EQ.0D0) CQSZ=1D0 + slPA=ATAN2(SQSZ,CQSZ) + + END |