mirror of
https://github.com/eddyem/BTA_lib.git
synced 2026-03-21 09:11:08 +03:00
copy
This commit is contained in:
100
slalib/tpv2c.f
Normal file
100
slalib/tpv2c.f
Normal file
@@ -0,0 +1,100 @@
|
||||
SUBROUTINE sla_TPV2C (XI, ETA, V, V01, V02, N)
|
||||
*+
|
||||
* - - - - - -
|
||||
* T P V 2 C
|
||||
* - - - - - -
|
||||
*
|
||||
* Given the tangent-plane coordinates of a star and its direction
|
||||
* cosines, determine the direction cosines of the tangent-point.
|
||||
*
|
||||
* (single precision)
|
||||
*
|
||||
* Given:
|
||||
* XI,ETA r tangent plane coordinates of star
|
||||
* V r(3) direction cosines of star
|
||||
*
|
||||
* Returned:
|
||||
* V01 r(3) direction cosines of tangent point, solution 1
|
||||
* V02 r(3) direction cosines of tangent point, solution 2
|
||||
* N i number of solutions:
|
||||
* 0 = no solutions returned (note 2)
|
||||
* 1 = only the first solution is useful (note 3)
|
||||
* 2 = both solutions are useful (note 3)
|
||||
*
|
||||
* Notes:
|
||||
*
|
||||
* 1 The vector V must be of unit length or the result will be wrong.
|
||||
*
|
||||
* 2 Cases where there is no solution can only arise near the poles.
|
||||
* For example, it is clearly impossible for a star at the pole
|
||||
* itself to have a non-zero XI value, and hence it is meaningless
|
||||
* to ask where the tangent point would have to be.
|
||||
*
|
||||
* 3 Also near the poles, cases can arise where there are two useful
|
||||
* solutions. The argument N indicates whether the second of the
|
||||
* two solutions returned is useful. N=1 indicates only one useful
|
||||
* solution, the usual case; under these circumstances, the second
|
||||
* solution can be regarded as valid if the vector V02 is interpreted
|
||||
* as the "over-the-pole" case.
|
||||
*
|
||||
* 4 This routine is the Cartesian equivalent of the routine sla_TPS2C.
|
||||
*
|
||||
* P.T.Wallace Starlink 5 June 1995
|
||||
*
|
||||
* 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., 59 Temple Place, Suite 330,
|
||||
* Boston, MA 02111-1307 USA
|
||||
*
|
||||
*-
|
||||
|
||||
IMPLICIT NONE
|
||||
|
||||
REAL XI,ETA,V(3),V01(3),V02(3)
|
||||
INTEGER N
|
||||
|
||||
REAL X,Y,Z,RXY2,XI2,ETA2P1,SDF,R2,R,C
|
||||
|
||||
|
||||
X=V(1)
|
||||
Y=V(2)
|
||||
Z=V(3)
|
||||
RXY2=X*X+Y*Y
|
||||
XI2=XI*XI
|
||||
ETA2P1=ETA*ETA+1.0
|
||||
SDF=Z*SQRT(XI2+ETA2P1)
|
||||
R2=RXY2*ETA2P1-Z*Z*XI2
|
||||
IF (R2.GT.0.0) THEN
|
||||
R=SQRT(R2)
|
||||
C=(SDF*ETA+R)/(ETA2P1*SQRT(RXY2*(R2+XI2)))
|
||||
V01(1)=C*(X*R+Y*XI)
|
||||
V01(2)=C*(Y*R-X*XI)
|
||||
V01(3)=(SDF-ETA*R)/ETA2P1
|
||||
R=-R
|
||||
C=(SDF*ETA+R)/(ETA2P1*SQRT(RXY2*(R2+XI2)))
|
||||
V02(1)=C*(X*R+Y*XI)
|
||||
V02(2)=C*(Y*R-X*XI)
|
||||
V02(3)=(SDF-ETA*R)/ETA2P1
|
||||
IF (ABS(SDF).LT.1.0) THEN
|
||||
N=1
|
||||
ELSE
|
||||
N=2
|
||||
END IF
|
||||
ELSE
|
||||
N=0
|
||||
END IF
|
||||
|
||||
END
|
||||
Reference in New Issue
Block a user