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pxform_c

Table of contents
Procedure
Abstract
Required_Reading
Keywords
Brief_I/O
Detailed_Input
Detailed_Output
Parameters
Exceptions
Files
Particulars
Examples
Restrictions
Literature_References
Author_and_Institution
Version
Index_Entries

Procedure

   pxform_c ( Position Transformation Matrix ) 

   void pxform_c ( ConstSpiceChar   * from,
                   ConstSpiceChar   * to,
                   SpiceDouble        et,
                   SpiceDouble        rotate[3][3] )

Abstract

   Return the matrix that transforms position vectors from one
   specified frame to another at a specified epoch.

Required_Reading

   FRAMES

Keywords

   FRAMES


Brief_I/O

   VARIABLE  I/O  DESCRIPTION
   --------  ---  --------------------------------------------------
   from       I   Name of the frame to transform from.
   to         I   Name of the frame to transform to.
   et         I   Epoch of the rotation matrix.
   rotate     O   A rotation matrix.

Detailed_Input

   from        is the name of a reference frame in which a position
               vector is known.

   to          is the name of a reference frame in which it is desired
               to represent a position vector.

   et          is the epoch in ephemeris seconds past the epoch of J2000
               (TDB) at which the position transformation matrix `rotate'
               should be evaluated.

Detailed_Output

   rotate      is the matrix that transforms position vectors from
               the reference frame `from' to the frame `to' at epoch `et'.
               If (x, y, z) is a position relative to the frame `from'
               then the vector ( x', y', z') is the same position
               relative to the frame `to' at epoch `et'. Here the
               vector ( x', y', z' ) is defined by the equation:

                  .-   -.     .-        -.   .-  -.
                  | x'  |     |          |   | x  |
                  | y'  |  =  |  rotate  |   | y  |
                  | z'  |     |          |   | z  |
                  `-   -'     `-        -'   `-  -'

Parameters

   None.

Exceptions

   1)  If sufficient information has not been supplied via loaded
       SPICE kernels to compute the transformation between the
       two frames, an error is signaled by a routine
       in the call tree of this routine.

   2)  If either frame `from' or `to' is not recognized, the error
       SPICE(UNKNOWNFRAME) is signaled by a routine in the call tree
       of this routine.

   3)  If any of the `from' or `to' input string pointers is null,
       the error SPICE(NULLPOINTER) is signaled.

   4)  If any of the `from' or `to' input strings has zero length,
       the error SPICE(EMPTYSTRING) is signaled.

Files

   None.

Particulars

   This routine provides the user level interface to computing
   position transformations from one reference frame to another.

   Note that the reference frames may be inertial or non-inertial.
   However, the user must take care that sufficient SPICE kernel
   information is loaded to provide a complete position
   transformation path from the `from' frame to the `to' frame.

   A common type of reference frame transformation is one from one
   time-dependent frame to another, where the orientations of the
   frames are computed at different epochs. For example, a remote
   sensing application may compute the transformation from a target
   body-fixed frame, with its orientation evaluated at the epoch of
   photon emission, to a spacecraft instrument frame, with its
   orientation evaluated at the epoch of photon reception. The
   CSPICE routine pxfrm2_c computes this type of frame
   transformation.

Examples

   Suppose that you have geodetic coordinates of a station on the
   surface of the earth and that you need the inertial (J2000)
   position of this station. The following code fragment
   illustrates how to transform the position of the station to a
   J2000 position.

      #include "SpiceUsr.h"
            .
            .
            .
      bodvcd_c ( 399, radii, 3, &n, abc );

      equatr   =  abc[0];
      polar    =  abc[2];
      f        =  ( equatr - polar ) / equatr;

      georec_c ( long,        lat,      0.0,   equatr,   f,   epos );
      pxform_c ( "IAU_EARTH", "J2000",  et,    rotate              );
      mxv_c    (  rotate,   epos,     jpos                         );

   The position jpos is the desired J2000 position of the station.

Restrictions

   None.

Literature_References

   None.

Author_and_Institution

   C.H. Acton          (JPL)
   N.J. Bachman        (JPL)
   J. Diaz del Rio     (ODC Space)
   B.V. Semenov        (JPL)
   W.L. Taber          (JPL)
   E.D. Wright         (JPL)

Version

   -CSPICE Version 1.0.5, 10-AUG-2021 (JDR) (NJB)

       Edited the header to comply with NAIF standard.

       Added entries #3 and #4 to -Exceptions section. Updated the
       -Particulars section to mention pxfrm2_c.

   -CSPICE Version 1.0.4, 27-FEB-2008 (BVS)

       Added FRAMES to the -Required_Reading section of the header.

   -CSPICE Version 1.0.3, 24-OCT-2005 (NJB)

       Header updates: example had invalid flattening factor
       computation; this was corrected. Reference to bodvar_c was
       replaced with reference to bodvcd_c.

   -CSPICE Version 1.0.2, 07-JAN-2004 (EDW)

       Trivial typo correction to example section.

   -CSPICE Version 1.0.1, 29-JUL-2003 (NJB) (CHA)

       Various header corrections were made.

   -CSPICE Version 1.0.0, 20-JUN-1999 (NJB) (WLT)

Index_Entries

   Find a position transformation matrix
Fri Dec 31 18:41:11 2021