EME2000 (J2000) to terrestrial frame vector transformation - DEPRECATED
[pos_ter,vel_ter,jacob] = CL_fr_J20002ter(cjd,pos_J2000 [,vel_J2000,ut1_utc,xp,yp,dPsi,dEps,conv_iers])
This function is deprecated.
Replacement function: CL_fr_convert
Converts position and (optionally) velocity vectors from EME2000 to the terrestrial ("Earth fixed") reference frame.
The jacobian of the transformation is optionally computed.
See Reference frames for more details on the definition of reference frames.
modified julian day from 1950.0 (UTC) (1xN or 1x1)
position vector relative to EME2000 [m] (3xN or 3x1)
(optional) velocity vector relative to EME2000 [m/s] (3xN or 3x1)
(optional) ut1-utc [seconds] (default is 0) (1xN or 1x1)
(optional) x polar coordinate [radians] (default is 0) (1xN or 1x1)
(optional) y polar coordinate [radians] (default is 0) (1xN or 1x1)
(optional) Nutation corrections [radians] (default is 0) (1xN or 1x1)
(optional) Nutation corrections [radians] (default is 0) (1xN or 1x1)
(optional) Convention IERS. Only iers 1996 (Lieske/Wahr) is implemented (default is "iers_1996")
position vector relative to terrestrial frame [m] (3xN)
(optional) velocity vector relative to terrestrial frame [m/s] (3xN)
(optional) jacobian of the transformation (6x6xN)
CNES - DCT/SB
1) IERS Conventions (1996), Dennis D. McCarthy
2) Explanatory Supplement to the Astronomical Almanac, Seidelman (1992)