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authorJoe Hunkeler <jhunkeler@gmail.com>2015-08-11 16:51:37 -0400
committerJoe Hunkeler <jhunkeler@gmail.com>2015-08-11 16:51:37 -0400
commit40e5a5811c6ffce9b0974e93cdd927cbcf60c157 (patch)
tree4464880c571602d54f6ae114729bf62a89518057 /math/slalib/ecor.f
downloadiraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz
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+ SUBROUTINE slECOR (RM, DM, IY, ID, FD, RV, TL)
+*+
+* - - - - -
+* E C O R
+* - - - - -
+*
+* Component of Earth orbit velocity and heliocentric
+* light time in a given direction (single precision)
+*
+* Given:
+* RM,DM real mean RA, Dec of date (radians)
+* IY int year
+* ID int day in year (1 = Jan 1st)
+* FD real fraction of day
+*
+* Returned:
+* RV real component of Earth orbital velocity (km/sec)
+* TL real component of heliocentric light time (sec)
+*
+* Notes:
+*
+* 1 The date and time is TDB (loosely ET) in a Julian calendar
+* which has been aligned to the ordinary Gregorian
+* calendar for the interval 1900 March 1 to 2100 February 28.
+* The year and day can be obtained by calling slCAYD or
+* slCLYD.
+*
+* 2 Sign convention:
+*
+* The velocity component is +ve when the Earth is receding from
+* the given point on the sky. The light time component is +ve
+* when the Earth lies between the Sun and the given point on
+* the sky.
+*
+* 3 Accuracy:
+*
+* The velocity component is usually within 0.004 km/s of the
+* correct value and is never in error by more than 0.007 km/s.
+* The error in light time correction is about 0.03s at worst,
+* but is usually better than 0.01s. For applications requiring
+* higher accuracy, see the slEVP and slEPV routines.
+*
+* Called: slERTH, slCS2C, slVDV
+*
+* Last revision: 5 April 2005
+*
+* Copyright P.T.Wallace. All rights reserved.
+*
+* 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
+
+ REAL RM,DM
+ INTEGER IY,ID
+ REAL FD,RV,TL
+
+ REAL slVDV
+
+ REAL PV(6),V(3),AUKM,AUSEC
+
+* AU to km and light sec (1985 Almanac)
+ PARAMETER (AUKM=1.4959787066E8,
+ : AUSEC=499.0047837)
+
+
+
+* Sun:Earth position & velocity vector
+ CALL slERTH(IY,ID,FD,PV)
+
+* Star position vector
+ CALL slCS2C(RM,DM,V)
+
+* Velocity component
+ RV=-AUKM*slVDV(PV(4),V)
+
+* Light time component
+ TL=AUSEC*slVDV(PV(1),V)
+
+ END