irfnam |
Table of contents
ProcedureIRFNAM ( Inertial reference frame name ) ENTRY IRFNAM ( INDEX, NAME ) AbstractReturn the name of one of the standard inertial reference frames supported by IRFROT. Required_ReadingFRAMES KeywordsCONVERSION COORDINATES EPHEMERIS FRAMES MATRIX ROTATION TRANSFORMATION VECTOR DeclarationsINTEGER INDEX CHARACTER*(*) NAME Brief_I/OVARIABLE I/O DESCRIPTION -------- --- -------------------------------------------------- INDEX I Index of standard inertial reference frame. NAME O Name of frame. Detailed_InputINDEX is the index of one of the standard inertial reference frames supported by IRFROT. Detailed_OutputNAME is the name of the frame specified by INDEX. ParametersNone. Exceptions1) If INDEX is not the index of a supported frame, NAME is blank. FilesNone. ParticularsIRFNAM is supplied as a convenience, to allow users to determine the names of standard inertial reference frames referred to only by index (as in the segment descriptors of a GEF ephemeris file). ExamplesIn the following example, the identity of a rotation from DE-118 to FK4 is deduced from the indices used to create the rotation. CALL IRFROT ( A, B, ROTAB ) CALL IRFNAM ( A, NAME(1) ) CALL IRFNAM ( B, NAME(2) ) WRITE (6,*) 'Rotation from ' // NAME(1) // ' to ' // NAME(2) Note that the name of the default reference frame can only be recovered from the number: CALL IRFNUM ( 'DEFAULT', DINDEX ) CALL IRFNAM ( DINDEX, DNAME ) RestrictionsNone. Literature_References[1] J. Lieske, "Precession Matrix Based on IAU (1976) System of Astronomical Constants," Astron. Astrophys. 73, 282-284, 1979. [2] E. M. Standish, Jr., "Orientation of the JPL Ephemerides, DE 200/LE 200, to the Dynamical Equinox of J2000," Astron. Astrophys. 114, 297-302, 1982. [3] E. M. Standish, Jr., "Conversion of Ephemeris Coordinates from the B1950 System to the J2000 System," JPL IOM 314.6-581, 24 June 1985. [4] E. M. Standish, Jr., "The Equinox Offsets of the JPL Ephemeris," JPL IOM 314.6-929, 26 February 1988. [5] J. Lieske, "Expressions for the Precession Quantities Based upon the IAU (1976) System of Astronomical Constants," Astron. Astrophys. 58, 1-16, 1977. [6] L. Bass and R. Cesarone, "Mars Observer Planetary Constants and Models," JPL D-3444, November 1990. [7] P. Kenneth Seidelmann (Ed.), "Explanatory Supplement to the Astronomical Almanac," University Science Books, 1992. Author_and_InstitutionJ. Diaz del Rio (ODC Space) W.L. Taber (JPL) I.M. Underwood (JPL) E.D. Wright (JPL) VersionSPICELIB Version 4.3.0, 17-JUN-2021 (JDR) Added IMPLICIT NONE statement. Edited the header to comply with NAIF standard. Added $Literature_References. SPICELIB Version 4.2.1, 04-JAN-2002 (EDW) Added DE-143 to header description for IRFROT. SPICELIB Version 4.2.0, 10-APR-1997 (WLT) A descriptive diagnostic was added to the entry points IRFROT and IRFDEF. Before they simply signaled the error with no diagnostic. SPICELIB Version 4.1.0, 14-OCT-1996 (WLT) The number of inertial frames recognized is now stored in the include file ninert.inc. SPICELIB Version 4.0.0, 20-MAY-1996 (WLT) The inertial frame DE-143 was added to the list of recognized inertial frames. SPICELIB Version 3.0.0, 20-MAR-1995 (WLT) The inertial frames DE-140 and DE-142 were added to the list of recognized inertial frames. SPICELIB Version 2.0.0, 30-JUL-1993 (WLT) The transformation from J2000 to B1950 was upgraded so that the transformation matrix produced matches the matrix given in [1]. The frame MARSIAU was added to the list of recognized frames. This is the standard mars referenced inertial frame used by the Mars Observer project. Values for the obliquity of the ecliptic were taken from the Explanatory Supplement [7] to the Astronomical Almanac (1992) at both the epochs J2000 and B1950 and used to define the mean ecliptic and equinox frames ECLIPJ2000 and ECLIPB1950. SPICELIB Version 1.0.1, 10-MAR-1992 (WLT) Comment section for permuted index source lines was added following the header. SPICELIB Version 1.0.0, 31-JAN-1990 (WLT) (IMU) |
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