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+.help evp Jun99 "Slalib Package"
+.nf
+
+ SUBROUTINE slEVP (DATE, DEQX, DVB, DPB, DVH, DPH)
+
+ - - - -
+ E V P
+ - - - -
+
+ Barycentric and heliocentric velocity and position of the Earth
+
+ All arguments are double precision
+
+ Given:
+
+ DATE TDB (loosely ET) as a Modified Julian Date
+ (JD-2400000.5)
+
+ DEQX Julian Epoch (e.g. 2000.0D0) of mean equator and
+ equinox of the vectors returned. If DEQX .LE. 0D0,
+ all vectors are referred to the mean equator and
+ equinox (FK5) of epoch DATE.
+
+ Returned (all 3D Cartesian vectors):
+
+ DVB,DPB barycentric velocity, position
+
+ DVH,DPH heliocentric velocity, position
+
+ (Units are AU/s for velocity and AU for position)
+
+ Called: slEPJ, slPREC
+
+ Accuracy:
+
+ The maximum deviations from the JPL DE96 ephemeris are as
+ follows:
+
+ barycentric velocity 0.42 m/s
+ barycentric position 6900 km
+
+ heliocentric velocity 0.42 m/s
+ heliocentric position 1600 km
+
+ This routine is adapted from the BARVEL and BARCOR
+ subroutines of P.Stumpff, which are described in
+ Astron. Astrophys. Suppl. Ser. 41, 1-8 (1980). Most of the
+ changes are merely cosmetic and do not affect the results at
+ all. However, some adjustments have been made so as to give
+ results that refer to the new (IAU 1976 'FK5') equinox
+ and precession, although the differences these changes make
+ relative to the results from Stumpff's original 'FK4' version
+ are smaller than the inherent accuracy of the algorithm. One
+ minor shortcoming in the original routines that has NOT been
+ corrected is that better numerical accuracy could be achieved
+ if the various polynomial evaluations were nested. Note also
+ that one of Stumpff's precession constants differs by 0.001 arcsec
+ from the value given in the Explanatory Supplement to the A.E.
+
+ P.T.Wallace Starlink 21 March 1999
+
+ Copyright (C) 1999 Rutherford Appleton Laboratory
+ Copyright (C) 1995 Association of Universities for Research in Astronomy Inc.
+
+.fi
+.endhelp