tipbod |
Table of contents
ProcedureTIPBOD ( Transformation, inertial position to bodyfixed ) SUBROUTINE TIPBOD ( REF, BODY, ET, TIPM ) AbstractReturn a 3x3 matrix that transforms positions in inertial coordinates to positions in body-equator-and-prime-meridian coordinates. Required_ReadingFRAMES PCK NAIF_IDS ROTATION TIME KeywordsROTATION TRANSFORMATION DeclarationsIMPLICIT NONE CHARACTER*(*) REF INTEGER BODY DOUBLE PRECISION ET DOUBLE PRECISION TIPM ( 3, 3 ) Brief_I/OVARIABLE I/O DESCRIPTION -------- --- -------------------------------------------------- REF I ID of inertial reference frame to transform from. BODY I ID code of body. ET I Epoch of transformation. TIPM O Position transformation matrix, inertial to prime meridian. Detailed_InputREF is the NAIF name for an inertial reference frame. Acceptable names include: Name Description -------- -------------------------------- 'J2000' Earth mean equator, dynamical equinox of J2000 'B1950' Earth mean equator, dynamical equinox of B1950 'FK4' Fundamental Catalog (4) 'DE-118' JPL Developmental Ephemeris (118) 'DE-96' JPL Developmental Ephemeris ( 96) 'DE-102' JPL Developmental Ephemeris (102) 'DE-108' JPL Developmental Ephemeris (108) 'DE-111' JPL Developmental Ephemeris (111) 'DE-114' JPL Developmental Ephemeris (114) 'DE-122' JPL Developmental Ephemeris (122) 'DE-125' JPL Developmental Ephemeris (125) 'DE-130' JPL Developmental Ephemeris (130) 'GALACTIC' Galactic System II 'DE-200' JPL Developmental Ephemeris (200) 'DE-202' JPL Developmental Ephemeris (202) See the Frames Required Reading frames.req for a full list of inertial reference frame names built into SPICE. The output TIPM will give the transformation from this frame to the bodyfixed frame specified by BODY at the epoch specified by ET. BODY is the integer ID code of the body for which the position transformation matrix is requested. Bodies are numbered according to the standard NAIF numbering scheme. The numbering scheme is explained in the NAIF IDs Required Reading naif_ids.req. ET is the epoch at which the position transformation matrix is requested. (This is typically the epoch of observation minus the one-way light time from the observer to the body at the epoch of observation.) Detailed_OutputTIPM is a 3x3 coordinate transformation matrix. It is used to transform positions from inertial coordinates to body fixed (also called equator and prime meridian --- PM) coordinates. Given a position P in the inertial reference frame specified by REF, the corresponding bodyfixed position is given by the matrix vector product: TIPM * S The X axis of the PM system is directed to the intersection of the equator and prime meridian. The Z axis points along the spin axis and points towards the same side of the invariable plane of the solar system as does earth's north pole. ParametersNone. Exceptions1) If the kernel pool does not contain all of the data required for computing the transformation matrix, TIPM, the error SPICE(INSUFFICIENTANGLES) is signaled. 2) If the reference frame, REF, is not recognized, an error is signaled by a routine in the call tree of this routine. 3) If the specified body code, BODY, is not recognized, an error is signaled by a routine in the call tree of this routine. FilesNone. ParticularsTIPBOD takes PCK information as input, either in the form of a binary or text PCK file. High precision binary files are searched for first (the last loaded file takes precedence); then it defaults to the text PCK file. If binary information is found for the requested body and time, the Euler angles are evaluated and the transformation matrix is calculated from them. Using the Euler angles PHI, DELTA and W we compute TIPM = [W] [DELTA] [PHI] 3 1 3 If no appropriate binary PCK files have been loaded, the text PCK file is used. Here information is found as RA, DEC and W (with the possible addition of nutation and libration terms for satellites). Again, the Euler angles are found, and the transformation matrix is calculated from them. The transformation from inertial to body-fixed coordinates is represented as: TIPM = [W] [HALFPI-DEC] [RA+HALFPI] 3 1 3 These are basically the Euler angles, PHI, DELTA and W: RA = PHI - HALFPI DEC = HALFPI - DELTA W = W The angles RA, DEC, and W are defined as follows in the text PCK file: 2 .----- RA1*t RA2*t \ RA = RA0 + ------- + ------- + ) a(i) * sin( theta(i) ) T 2 / T '----- i 2 .----- DEC1*t DEC2*t \ DEC = DEC0 + -------- + -------- + ) d(i) * cos( theta(i) ) T 2 / T '----- i 2 .----- W1*t W2*t \ W = W0 + ------ + ------- + ) w(i) * sin( theta(i) ) d 2 / d '----- i where `d' is in seconds/day; T in seconds/Julian century; a(i), d(i), and w(i) arrays apply to satellites only; and theta(i), defined as THETA1(i)*t theta(i) = THETA0(i) + ------------- T are specific to each planet. These angles ---typically nodal rates--- vary in number and definition from one planetary system to the next. 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) Calculate the matrix to rotate a position vector from the J2000 frame to the Saturn fixed frame at a specified time, and use it to compute the position of Titan in Saturn's body-fixed frame. Use the meta-kernel shown below to load the required SPICE kernels. KPL/MK File name: tipbod_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 --------- -------- sat375.bsp Saturn satellite ephemeris pck00010.tpc Planet orientation and radii naif0012.tls Leapseconds \begindata KERNELS_TO_LOAD = ( 'sat375.bsp', 'pck00010.tpc', 'naif0012.tls' ) \begintext End of meta-kernel Example code begins here. PROGRAM TIPBOD_EX1 IMPLICIT NONE C C Local variables C DOUBLE PRECISION ET DOUBLE PRECISION LT DOUBLE PRECISION POS ( 3 ) DOUBLE PRECISION SATVEC ( 3 ) DOUBLE PRECISION TIPM ( 3, 3 ) INTEGER SATID C C Load the kernels. C CALL FURNSH ( 'tipbod_ex1.tm' ) C C The body ID for Saturn. C SATID = 699 C C Retrieve the transformation matrix at some time. C CALL STR2ET ( 'Jan 1 2005', ET ) CALL TIPBOD ( 'J2000', SATID, ET, TIPM ) C C Retrieve the position of Titan as seen from Saturn C in the J2000 frame at ET. C CALL SPKPOS ( 'TITAN', ET, 'J2000', 'NONE', . 'SATURN', POS, LT ) WRITE(*,'(A)') 'Titan as seen from Saturn:' WRITE(*,'(A,3F13.3)') ' in J2000 frame :', POS C C Rotate the position 3-vector POS into the C Saturn body-fixed reference frame. C CALL MXV ( TIPM, POS, SATVEC ) WRITE(*,'(A,3F13.3)') ' in IAU_SATURN frame:', SATVEC END When this program was executed on a Mac/Intel/gfortran/64-bit platform, the output was: Titan as seen from Saturn: in J2000 frame : 1071928.661 -505781.970 -60383.976 in IAU_SATURN frame: 401063.338 -1116965.364 -5408.806 Note that the complete example could be replaced by a single SPKPOS call: CALL SPKPOS ( 'TITAN', ET, 'IAU_SATURN', 'NONE', . 'SATURN', POS, LT ) Restrictions1) The kernel pool must be loaded with the appropriate coefficients (from a text or binary PCK file) prior to calling this routine. Literature_ReferencesNone. Author_and_InstitutionN.J. Bachman (JPL) J. Diaz del Rio (ODC Space) H.A. Neilan (JPL) B.V. Semenov (JPL) W.L. Taber (JPL) K.S. Zukor (JPL) VersionSPICELIB Version 1.4.0, 06-JUL-2021 (JDR) Added IMPLICIT NONE statement. Edited the header to comply with NAIF standard. Removed unnecessary entries in $Revisions section. Added complete code example. Added frames.req to $Required_Reading. SPICELIB Version 1.3.0, 02-MAR-2016 (BVS) Updated to use the 3x3 top-left corner of the 6x6 matrix returned by TISBOD instead of fetching kernel data and doing computations in-line. Fixed indentation of some header sections. SPICELIB Version 1.2.0, 23-OCT-2005 (NJB) Updated to remove non-standard use of duplicate arguments in MXM call. Replaced header references to LDPOOL with references to FURNSH. SPICELIB Version 1.1.0, 05-JAN-2005 (NJB) Tests of routine FAILED() were added. SPICELIB Version 1.0.3, 10-MAR-1994 (KSZ) Underlying BODMAT code changed to look for binary PCK data files, and use them to get orientation information if they are available. Only the comments to TIPBOD changed. SPICELIB Version 1.0.2, 06-JUL-1993 (HAN) Example in header was corrected. Previous version had incorrect matrix dimension specifications passed to MXVG. 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, 05-AUG-1991 (NJB) (WLT) |
Fri Dec 31 18:37:02 2021