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/dh2e.f
Normal file
100
slalib/dh2e.f
Normal file
@@ -0,0 +1,100 @@
|
||||
SUBROUTINE sla_DH2E (AZ, EL, PHI, HA, DEC)
|
||||
*+
|
||||
* - - - - -
|
||||
* D E 2 H
|
||||
* - - - - -
|
||||
*
|
||||
* Horizon to equatorial coordinates: Az,El to HA,Dec
|
||||
*
|
||||
* (double precision)
|
||||
*
|
||||
* Given:
|
||||
* AZ d azimuth
|
||||
* EL d elevation
|
||||
* PHI d observatory latitude
|
||||
*
|
||||
* Returned:
|
||||
* HA d hour angle
|
||||
* DEC d declination
|
||||
*
|
||||
* Notes:
|
||||
*
|
||||
* 1) All the arguments are angles in radians.
|
||||
*
|
||||
* 2) The sign convention for azimuth is north zero, east +pi/2.
|
||||
*
|
||||
* 3) HA is returned in the range +/-pi. Declination is returned
|
||||
* in the range +/-pi/2.
|
||||
*
|
||||
* 4) The latitude is (in principle) geodetic. In critical
|
||||
* applications, corrections for polar motion should be applied.
|
||||
*
|
||||
* 5) In some applications it will be important to specify the
|
||||
* correct type of elevation in order to produce the required
|
||||
* type of HA,Dec. In particular, it may be important to
|
||||
* distinguish between the elevation as affected by refraction,
|
||||
* which will yield the "observed" HA,Dec, and the elevation
|
||||
* in vacuo, which will yield the "topocentric" HA,Dec. If the
|
||||
* effects of diurnal aberration can be neglected, the
|
||||
* topocentric HA,Dec may be used as an approximation to the
|
||||
* "apparent" HA,Dec.
|
||||
*
|
||||
* 6) No range checking of arguments is done.
|
||||
*
|
||||
* 7) In applications which involve many such calculations, rather
|
||||
* than calling the present routine it will be more efficient to
|
||||
* use inline code, having previously computed fixed terms such
|
||||
* as sine and cosine of latitude.
|
||||
*
|
||||
* P.T.Wallace Starlink 21 February 1996
|
||||
*
|
||||
* Copyright (C) 1996 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
|
||||
|
||||
DOUBLE PRECISION AZ,EL,PHI,HA,DEC
|
||||
|
||||
DOUBLE PRECISION SA,CA,SE,CE,SP,CP,X,Y,Z,R
|
||||
|
||||
|
||||
* Useful trig functions
|
||||
SA=SIN(AZ)
|
||||
CA=COS(AZ)
|
||||
SE=SIN(EL)
|
||||
CE=COS(EL)
|
||||
SP=SIN(PHI)
|
||||
CP=COS(PHI)
|
||||
|
||||
* HA,Dec as x,y,z
|
||||
X=-CA*CE*SP+SE*CP
|
||||
Y=-SA*CE
|
||||
Z=CA*CE*CP+SE*SP
|
||||
|
||||
* To HA,Dec
|
||||
R=SQRT(X*X+Y*Y)
|
||||
IF (R.EQ.0D0) THEN
|
||||
HA=0D0
|
||||
ELSE
|
||||
HA=ATAN2(Y,X)
|
||||
END IF
|
||||
DEC=ATAN2(Z,R)
|
||||
|
||||
END
|
||||
Reference in New Issue
Block a user