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slalib/refco.f

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+      SUBROUTINE sla_REFCO ( HM, TDK, PMB, RH, WL, PHI, TLR, EPS,
+     :                       REFA, REFB )
+*+
+*     - - - - - -
+*      R E F C O
+*     - - - - - -
+*
+*  Determine the constants A and B in the atmospheric refraction
+*  model dZ = A tan Z + B tan**3 Z.
+*
+*  Z is the "observed" zenith distance (i.e. affected by refraction)
+*  and dZ is what to add to Z to give the "topocentric" (i.e. in vacuo)
+*  zenith distance.
+*
+*  Given:
+*    HM      d     height of the observer above sea level (metre)
+*    TDK     d     ambient temperature at the observer (K)
+*    PMB     d     pressure at the observer (millibar)
+*    RH      d     relative humidity at the observer (range 0-1)
+*    WL      d     effective wavelength of the source (micrometre)
+*    PHI     d     latitude of the observer (radian, astronomical)
+*    TLR     d     temperature lapse rate in the troposphere (K/metre)
+*    EPS     d     precision required to terminate iteration (radian)
+*
+*  Returned:
+*    REFA    d     tan Z coefficient (radian)
+*    REFB    d     tan**3 Z coefficient (radian)
+*
+*  Called:  sla_REFRO
+*
+*  Notes:
+*
+*  1  Typical values for the TLR and EPS arguments might be 0.0065D0 and
+*     1D-10 respectively.
+*
+*  2  The radio refraction is chosen by specifying WL > 100 micrometres.
+*
+*  3  The routine is a slower but more accurate alternative to the
+*     sla_REFCOQ routine.  The constants it produces give perfect
+*     agreement with sla_REFRO at zenith distances arctan(1) (45 deg)
+*     and arctan(4) (about 76 deg).  It achieves 0.5 arcsec accuracy
+*     for ZD < 80 deg, 0.01 arcsec accuracy for ZD < 60 deg, and
+*     0.001 arcsec accuracy for ZD < 45 deg.
+*
+*  P.T.Wallace   Starlink   22 May 2004
+*
+*  Copyright (C) 2004 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 HM,TDK,PMB,RH,WL,PHI,TLR,EPS,REFA,REFB
+
+      DOUBLE PRECISION ATN1,ATN4,R1,R2
+
+*  Sample zenith distances: arctan(1) and arctan(4)
+      PARAMETER (ATN1=0.7853981633974483D0,
+     :           ATN4=1.325817663668033D0)
+
+
+
+*  Determine refraction for the two sample zenith distances
+      CALL sla_REFRO(ATN1,HM,TDK,PMB,RH,WL,PHI,TLR,EPS,R1)
+      CALL sla_REFRO(ATN4,HM,TDK,PMB,RH,WL,PHI,TLR,EPS,R2)
+
+*  Solve for refraction constants
+      REFA = (64D0*R1-R2)/60D0
+      REFB = (R2-4D0*R1)/60D0
+
+      END