ckfrot |
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ProcedureCKFROT ( CK frame, find position rotation ) SUBROUTINE CKFROT ( INST, ET, ROTATE, REF, FOUND ) AbstractFind the position rotation matrix from a C-kernel (CK) frame with the specified frame class ID (CK ID) to the base frame of the highest priority CK segment containing orientation data for this CK frame at the time requested. Required_ReadingCK KeywordsPOINTING DeclarationsIMPLICIT NONE INTEGER INST DOUBLE PRECISION ET DOUBLE PRECISION ROTATE ( 3, 3 ) INTEGER REF LOGICAL FOUND Brief_I/OVARIABLE I/O DESCRIPTION -------- --- -------------------------------------------------- INST I Frame class ID (CK ID) of a CK frame. ET I Epoch measured in seconds past J2000 TDB. ROTATE O Rotation matrix from CK frame to frame REF. REF O Frame ID of the base reference. FOUND O .TRUE. when requested pointing is available. Detailed_InputINST is the unique frame class ID (CK ID) of the CK frame for which data is being requested. ET is the epoch for which the position rotation is desired. ET should be given in seconds past the epoch of J2000 TDB. Detailed_OutputROTATE is a position rotation matrix that converts positions relative to the CK frame given by its frame class ID, INST, to positions relative to the base frame given by its frame ID, REF. Thus, if a position S has components x,y,z in the CK frame, then S has components x', y', z' in the base frame. .- -. .- -. .- -. | x' | | | | x | | y' | = | ROTATE | | y | | z' | | | | z | `- -' `- -' `- -' REF is the ID code of the base reference frame to which ROTATE will transform positions. FOUND is .TRUE. if a record was found to satisfy the pointing request. FOUND will be .FALSE. otherwise. ParametersNone. Exceptions1) If no CK files were loaded prior to calling this routine, an error is signaled by a routine in the call tree of this routine. 2) If no SCLK correlation data needed to read CK files were loaded prior to calling this routine, an error is signaled by a routine in the call tree of this routine. 3) If the input time ET cannot be converted to an encoded SCLK time, using SCLK data associated with INST, an error is signaled by a routine in the call tree of this routine. FilesCKFROT searches through loaded CK files to locate a segment that can satisfy the request for position rotation data for the CK frame with the specified frame class ID at time ET. You must load a CK file containing such data before calling this routine. You must also load SCLK and possibly LSK files needed to convert the input ET time to the encoded SCLK time with which the orientation data stored inside that CK is tagged. ParticularsCKFROT searches through loaded CK files to satisfy a pointing request. Last-loaded files are searched first, and individual files are searched in backwards order, giving priority to segments that were added to a file later than the others. The search ends when a segment is found that can give pointing for the specified CK frame at the request time. Segments with and without angular velocities are considered by this routine. This routine uses the CKMETA routine to determine the SCLK ID used to convert the input ET time to the encoded SCLK time used to look up pointing data in loaded CK files. ExamplesThe numerical results shown for this example may differ across platforms. The results depend on the SPICE kernels used as input, the compiler and supporting libraries, and the machine specific arithmetic implementation. 1) Use CKFROT to compute the instantaneous angular velocity vector for the Mars Global Surveyor (MGS) spacecraft frame, 'MGS_SPACECRAFT', relative to the inertial frame used as the base frame in CK files containing MGS spacecraft orientation at 2003-JUL-25 13:00:00. The frame class ID (CK ID) for the 'MGS_SPACECRAFT' frame is -94000. Suppose that R(t) is the rotation matrix whose columns represent the inertial pointing vectors of the MGS spacecraft axes at time `t'. Then the angular velocity vector points along the vector given by: T limit AXIS( R(t+h)R ) h-->0 And the magnitude of the angular velocity at time `t' is given by: T d ANGLE ( R(t+h)R(t) ) ------------------------ at h = 0 dh Use the meta-kernel shown below to load the required SPICE kernels. KPL/MK File name: ckfrot_ex1.tm This meta-kernel is intended to support operation of SPICE example programs. The kernels shown here should not be assumed to contain adequate or correct versions of data required by SPICE-based user applications. In order for an application to use this meta-kernel, the kernels referenced here must be present in the user's current working directory. The names and contents of the kernels referenced by this meta-kernel are as follows: File name Contents --------- -------- naif0012.tls Leapseconds mgs_sclkscet_00061.tsc MGS SCLK coefficients mgs_sc_ext12.bc MGS s/c bus attitude \begindata KERNELS_TO_LOAD = ( 'naif0012.tls', 'mgs_sclkscet_00061.tsc', 'mgs_sc_ext12.bc' ) \begintext End of meta-kernel Example code begins here. PROGRAM CKFROT_EX1 IMPLICIT NONE C C Local parameters. C CHARACTER*(*) EPOCH PARAMETER ( EPOCH = '2003-JUL-25 13:00:00' ) INTEGER INST PARAMETER ( INST = -94000 ) C C Local variables. C DOUBLE PRECISION ANGLE DOUBLE PRECISION ANGVEL ( 3 ) DOUBLE PRECISION AXIS ( 3 ) DOUBLE PRECISION ET DOUBLE PRECISION INFROT ( 3, 3 ) DOUBLE PRECISION H DOUBLE PRECISION RET ( 3, 3 ) DOUBLE PRECISION RETH ( 3, 3 ) INTEGER REF INTEGER REFH LOGICAL FOUND LOGICAL FOUNDH C C Load the required LSK, SCLK and CK. Use a C meta-kernel for convenience. C CALL FURNSH ( 'ckfrot_ex1.tm' ) C C First convert the time to seconds past J2000. Set the C delta time (1 ms). C CALL STR2ET ( EPOCH, ET ) H = 1.D-3 C C Now, look up the rotation from the MGS spacecraft C frame specified by its frame class ID (CK ID) to a C base reference frame (returned by CKFROT), at ET C and ET+H. C CALL CKFROT ( INST, ET, RET, REF, FOUND ) CALL CKFROT ( INST, ET+H, RETH, REFH, FOUNDH ) C C If both rotations were computed and if the base C reference frames are the same, compute the C instantaneous angular velocity vector. C IF ( FOUND .AND. FOUNDH .AND. REF .EQ. REFH ) THEN C C Compute the infinitesimal rotation R(t+h)R(t)**T. C CALL MXMT ( RETH, RET, INFROT ) C C Compute the AXIS and ANGLE of the infinitesimal C rotation. C CALL RAXISA ( INFROT, AXIS, ANGLE ) C C Scale AXIS to get the angular velocity vector. C CALL VSCL ( ANGLE/H, AXIS, ANGVEL ) C C Output the results. C WRITE(*,'(A)') . 'Instantaneous angular velocity vector:' WRITE(*,'(3F15.10)') ANGVEL WRITE(*,'(A,I5)') 'Reference frame ID:', REF ELSE WRITE(*,*) 'ERROR: data not found or frame mismatch.' END IF END When this program was executed on a Mac/Intel/gfortran/64-bit platform, the output was: Instantaneous angular velocity vector: 0.0001244121 0.0008314866 0.0003028634 Reference frame ID: 1 Restrictions1) A CK file must be loaded prior to calling this routine. 2) LSK and SCLK files needed for time conversions must be loaded prior to calling this routine. Literature_ReferencesNone. Author_and_InstitutionJ. Diaz del Rio (ODC Space) B.V. Semenov (JPL) W.L. Taber (JPL) VersionSPICELIB Version 1.3.0, 13-DEC-2021 (JDR) (BVS) (NJB) Edited the header to comply with NAIF standard and modern SPICE CK and frames terminology. Added initialization of local variable SFND. Added complete code example. SPICELIB Version 1.2.0, 17-FEB-2000 (WLT) The routine now checks to make sure convert ET to TICKS and that at least one C-kernel is loaded before trying to look up the transformation. Also the routine now calls SCE2C instead of SCE2T. SPICELIB Version 1.0.0, 03-MAR-1999 (WLT) |
Fri Dec 31 18:36:02 2021