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author | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
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committer | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
commit | fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4 (patch) | |
tree | bdda434976bc09c864f2e4fa6f16ba1952b1e555 /math/slalib/hfk5z.f | |
download | iraf-linux-fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4.tar.gz |
Initial commit
Diffstat (limited to 'math/slalib/hfk5z.f')
-rw-r--r-- | math/slalib/hfk5z.f | 140 |
1 files changed, 140 insertions, 0 deletions
diff --git a/math/slalib/hfk5z.f b/math/slalib/hfk5z.f new file mode 100644 index 00000000..2f6d53b2 --- /dev/null +++ b/math/slalib/hfk5z.f @@ -0,0 +1,140 @@ + SUBROUTINE slHF5Z (RH,DH,EPOCH,R5,D5,DR5,DD5) +*+ +* - - - - - - +* H F 5 Z +* - - - - - - +* +* Transform a Hipparcos star position into FK5 J2000, assuming +* zero Hipparcos proper motion. +* +* (double precision) +* +* Given: +* RH d Hipparcos RA (radians) +* DH d Hipparcos Dec (radians) +* EPOCH d Julian epoch (TDB) +* +* Returned (all FK5, equinox J2000, epoch EPOCH): +* R5 d RA (radians) +* D5 d Dec (radians) +* +* Called: slDS2C, slDAVM, slDMXV, slDMXM, +* slDIMV, slDVXV, slDC6S, slDA2P +* +* Notes: +* +* 1) The proper motion in RA is dRA/dt rather than cos(Dec)*dRA/dt. +* +* 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) It was the intention that Hipparcos should be a close +* approximation to an inertial frame, so that distant objects +* have zero proper motion; such objects have (in general) +* non-zero proper motion in FK5, and this routine returns those +* fictitious proper motions. +* +* 5) The position returned by this routine is in the FK5 J2000 +* reference frame but at Julian epoch EPOCH. +* +* 6) See also slFK5H, slHFK5, sla_FK5ZHZ. +* +* Reference: +* +* M.Feissel & F.Mignard, Astron. Astrophys. 331, L33-L36 (1998). +* +* P.T.Wallace Starlink 30 December 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 RH,DH,EPOCH,R5,D5,DR5,DD5 + + 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 PH(3),ORTN(3),R5H(3,3),S5(3),SH(3),T,VST(3), + : RST(3,3),R5HT(3,3),PV5E(6),VV(3),W,R,V + + DOUBLE PRECISION slDA2P + + + +* Hipparcos barycentric position vector (normalized). + CALL slDS2C(RH,DH,PH) + +* 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 + +* Rotate the spin vector into the Hipparcos frame. + CALL slDMXV(R5H,S5,SH) + +* Time interval from J2000 to epoch. + T = EPOCH-2000D0 + +* Axial vector: accumulated Hipparcos wrt FK5 spin over that interval. + VST(1) = OMX*T + VST(2) = OMY*T + VST(3) = OMZ*T + +* Express the accumulated spin as a rotation matrix. + CALL slDAVM(VST,RST) + +* Rotation matrix: accumulated spin, then FK5 to Hipparcos. + CALL slDMXM(R5H,RST,R5HT) + +* De-orient & de-spin the vector into FK5 J2000 at epoch. + CALL slDIMV(R5HT,PH,PV5E) + CALL slDVXV(SH,PH,VV) + CALL slDIMV(R5HT,VV,PV5E(4)) + +* FK5 position/velocity 6-vector to spherical. + CALL slDC6S(PV5E,W,D5,R,DR5,DD5,V) + R5 = slDA2P(W) + + END |