SailEphemJPL:

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   Location of planets relative to Sun in ecliptic frame using JPL ephemerides.
   This function fixes the moon position to be heliocentric from geocentric.
   If you are using the Moon you should be using the Earth too. The function
   PlanetPosJPL must be initialized with the desired planet IDs before
   calling this function.
   This format is for use with FSailCombined.
   See also PlanetPosJPL.

   Since version 7.
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   Form:
   rB = SailEphemJPL( jD, d )
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   Inputs
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   jD        (1,1)     Julian date.
   d          (:)      Data structure.
                       .kP   Array of planet IDs

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   Outputs
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   rB        (3,:)     Position of planets

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Children:

SC: Ephem/PlanetPosJPL