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: http://www.stsci.edu/~sontag/spicedocs/cspice/sct2e_c.html
Дата изменения: Sat Dec 17 06:09:40 2005 Дата индексирования: Sun Apr 10 23:27:36 2016 Кодировка: |
Convert encoded spacecraft clock (`ticks') to ephemeris seconds past J2000 (ET).
SCLK TIME
Variable I/O Description -------- --- -------------------------------------------------- sc I NAIF spacecraft ID code. sclkdp I SCLK, encoded as ticks since spacecraft clock start. et O Ephemeris time, seconds past J2000.
sc is a NAIF integer code for a spacecraft, one of whose encoded clock values is represented by sclkdp. sclkdp is an encoded spacecraft clock value. sclkdp represents time measured from spacecraft clock start: partition information IS reflected in the encoded value.
et is the epoch, specified as ephemeris seconds past J2000, that corresponds to sclkdp.
None.
This routine operates on encoded SCLK values. These values are obtained by calling the CSPICE routine scencd_c or other SCLK conversion routines. The advantage of encoded SCLK, as opposed to character string representations of SCLK is that encoded SCLK values are easy to perform arithmetic operations on. Additionally, working with encoded SCLK reduces the overhead of repeated conversion of character strings to integers or double precision numbers. To convert a string representation of an SCLK value to ET, use the CSPICE routine scs2e_c.
1) Encode a Galileo SCLK string, and convert the encoded value to ET; use these time values to look up both GLL orbiter scan platform's pointing and the GLL--Earth state vector for an epoch specified by an SCLK string. During program initialization, load the leapseconds and SCLK kernels. We will pretend that these files are named "leapseconds.ker" and "gllsclk.ker". To use this code fragment, you must substitute the actual names of these kernel files for the names used here. /. load leapseconds and sclk kernels: ./ ldpool_c ( "leapseconds.ker" ); ldpool_c ( "gllsclk.ker" ); /. The mission is Galileo, which has spacecraft ID -77. Let's assume that the SCLK string is 1 / 1900000:00:00 The number 1, followed by a slash, indicates that the epoch is in the first partition. The next step is to encode this SCLK string, and also find the corresponding ET value: ./ scencd_c ( -77, "1/ 1900000:00:00", &sclkdp ); sct2e_c ( -77, sclkdp, &et ); We'll assume that you've already loaded SPK and CK files containing ephemeris data for the GLL orbiter and the Earth, as well as scan platform pointing. Now you're ready to call both ckgp_c, which expects the input epoch to be specified by an encoded SCLK string, and spkez_c, which expects the epoch to be specified as an ephemeris time. /. Find scan platform pointing cmat and s/c--target vector (first 3 components of state) at epoch. We assume that CK and SPK kernels have been loaded already, via cklpf_c and spklef_c respectively. Use tolerance of 80 ticks for the CK look-up. ./ scanpl = -77001; earth = 399; tol = 80.0; ckgp_c ( scanpl, sclkdp, tol, refsys, cmat, &clkout, &found ); if ( !found ) { [ Indicate to user that pointing was not available ] } spkez_c ( earth, et, refsys, corr, -77, state, < ); 2) Convert an encoded Voyager 2 SCLK value to UTC, using calendar format, with 3 digits of precision. Again, your initialization code must load the leapseconds and SCLK kernels: /. load leapseconds and SCLK kernels: ./ ldpool_c ( "leapseconds.ker" ); ldpool_c ( "vgr2sclk.ker" ); To find the UTC value corresponding to the encoded Voyager 2 SCLK value sclkdp, you can use the code fragment sct2e_c ( -32, sclkdp, &et ); et2utc_c ( et, "c", 3, UTCLEN, utc ); where UTCLEN is a constant indicating the available room in the string utc. A value of 25 characters suffices.
1) An SCLK kernel appropriate to the spacecraft clock identified by SC must be loaded at the time this routine is called. 2) If the SCLK kernel used with this routine does not map SCLK directly to barycentric dynamical time, a leapseconds kernel must be loaded at the time this routine is called.
1) This routine assumes that that an SCLK kernel appropriate to the spacecraft clock identified by the input argument sc has been loaded. If an SCLK kernel has not been loaded, does not contain all of the required data, or contains invalid data, error diagnoses will be performed by routines called by this routine. The output argument et will not be modified. 2) When using SCLK kernels that map SCLK to a time system other than ET (also called barycentric dynamical time---`TDB'), it is necessary to have a leapseconds kernel loaded at the time this routine is called. If a leapseconds kernel is required for conversion between SCLK and ET but is not loaded, the error will be diagnosed by routines called by this routine. The output argument et will not be modified. The time system that an SCLK kernel maps SCLK to is indicated by the variable SCLK_TIME_SYSTEM_nn in the kernel, where nn is the negative of the NAIF integer code for the spacecraft. The time system used in a kernel is TDB if and only if the variable is assigned the value 1. 3) If the clock type for the spacecraft clock identified by sc is not supported by this routine, the error SPICE(NOTSUPPORTED) is signalled. The output argument et will not be modified. 4) If the input argument sclkdp is invalid, the error will be diagnosed by routines called by this routine. The output argument et will not be modified.
None.
N.J. Bachman (JPL)
[1] CK Required Reading [2] SPK Required Reading
-CSPICE Version 1.0.0, 08-FEB-1998 (NJB) Based on SPICELIB Version 1.0.2, 10-APR-1992 (NJB) (WLT)
spacecraft_clock ticks to ephemeris time