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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/doc/pa.hlp | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'math/slalib/doc/pa.hlp')
-rw-r--r-- | math/slalib/doc/pa.hlp | 36 |
1 files changed, 36 insertions, 0 deletions
diff --git a/math/slalib/doc/pa.hlp b/math/slalib/doc/pa.hlp new file mode 100644 index 00000000..a7ee7357 --- /dev/null +++ b/math/slalib/doc/pa.hlp @@ -0,0 +1,36 @@ +.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 |