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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/fk52h.f | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'math/slalib/fk52h.f')
-rw-r--r-- | math/slalib/fk52h.f | 123 |
1 files changed, 123 insertions, 0 deletions
diff --git a/math/slalib/fk52h.f b/math/slalib/fk52h.f new file mode 100644 index 00000000..4d9d42f8 --- /dev/null +++ b/math/slalib/fk52h.f @@ -0,0 +1,123 @@ + SUBROUTINE slFK5H (R5,D5,DR5,DD5,RH,DH,DRH,DDH) +*+ +* - - - - - - +* F K 5 H +* - - - - - - +* +* Transform FK5 (J2000) star data into the Hipparcos frame. +* +* (double precision) +* +* This routine transforms FK5 star positions and proper motions +* into the frame of the Hipparcos catalogue. +* +* Given (all FK5, equinox J2000, epoch J2000): +* R5 d RA (radians) +* D5 d Dec (radians) +* DR5 d proper motion in RA (dRA/dt, rad/Jyear) +* DD5 d proper motion in Dec (dDec/dt, rad/Jyear) +* +* Returned (all Hipparcos, epoch J2000): +* RH d RA (radians) +* DH d Dec (radians) +* DRH d proper motion in RA (dRA/dt, rad/Jyear) +* DDH d proper motion in Dec (dDec/dt, rad/Jyear) +* +* Called: slDSC6, slDAVM, slDMXV, slDVXV, slDC6S, +* slDA2P +* +* Notes: +* +* 1) The proper motions in RA are dRA/dt rather than +* cos(Dec)*dRA/dt, and are per year rather than per century. +* +* 2) The FK5 to Hipparcos transformation consists of a pure +* rotation and spin; zonal errors in the FK5 catalogue are +* not taken into account. +* +* 3) The published orientation and spin components are interpreted +* as "axial vectors". An axial vector points at the pole of the +* rotation and its length is the amount of rotation in radians. +* +* 4) See also slHFK5, slF5HZ, slHF5Z. +* +* Reference: +* +* M.Feissel & F.Mignard, Astron. Astrophys. 331, L33-L36 (1998). +* +* P.T.Wallace Starlink 22 June 1999 +* +* Copyright (C) 1999 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 R5,D5,DR5,DD5,RH,DH,DRH,DDH + + DOUBLE PRECISION AS2R + PARAMETER (AS2R=0.484813681109535994D-5) + +* FK5 to Hipparcos orientation and spin (radians, radians/year) + DOUBLE PRECISION EPX,EPY,EPZ + DOUBLE PRECISION OMX,OMY,OMZ + + PARAMETER ( EPX = -19.9D-3 * AS2R, + : EPY = -9.1D-3 * AS2R, + : EPZ = +22.9D-3 * AS2R ) + + PARAMETER ( OMX = -0.30D-3 * AS2R, + : OMY = +0.60D-3 * AS2R, + : OMZ = +0.70D-3 * AS2R ) + + DOUBLE PRECISION PV5(6),ORTN(3),R5H(3,3),S5(3),VV(3),PVH(6),W,R,V + INTEGER I + + DOUBLE PRECISION slDA2P + + + +* FK5 barycentric position/velocity 6-vector (normalized). + CALL slDSC6(R5,D5,1D0,DR5,DD5,0D0,PV5) + +* FK5 to Hipparcos orientation matrix. + ORTN(1) = EPX + ORTN(2) = EPY + ORTN(3) = EPZ + CALL slDAVM(ORTN,R5H) + +* Hipparcos wrt FK5 spin vector. + S5(1) = OMX + S5(2) = OMY + S5(3) = OMZ + +* Orient & spin the 6-vector into the Hipparcos frame. + CALL slDMXV(R5H,PV5,PVH) + CALL slDVXV(PV5,S5,VV) + DO I=1,3 + VV(I) = PV5(I+3)+VV(I) + END DO + CALL slDMXV(R5H,VV,PVH(4)) + +* Hipparcos 6-vector to spherical. + CALL slDC6S(PVH,W,DH,R,DRH,DDH,V) + RH = slDA2P(W) + + END |