PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT INTERCHANGE_FORMAT = ASCII PUBLICATION_DATE = 2010-03-15 NOTE = "SCL-Kernel Information" END_OBJECT = TEXT END General Information About SPICE SCL-Kernels =========================================== In the SPICE system, Spacecraft Clock (or SCL) -kernel contains a set of information required to perform a mapping between Ephemeris time (ET) and spacecraft on-board time (SCLK). The spacecraft clock coefficient information contained in SCLK file can be manipulated using the SPICE Toolkit APIs, calls to which can be integrated into user application programs. The information regarding how to obtain the SPICE system toolkit for a number of languages and computer platforms is located in the ``/software'' subdirectory of the main directory of this data set. Refer to the ``sclk.req'' document provided with the toolkit to get more information about conversion between ET and spacecraft clock times. MESSENGER SCL-kernels Contained in This Data Set ================================================ This data set contains the following MESSENGER SCLK files (only name portion of the file name is shown on the right; the extension of all file names is ``.tsc''): messenger_[VER] MESSENGER Spacecraft clock coefficients Kernel (SCLK) files containing actual MESSENGER on-board clock to ET mapping coefficients computed using time calibration packets from the spacecraft engineering telemetry. If this data set contains multiple SCLK files, the one with the latest version ([VER]) supersedes all previous versions. Kernel File Details =================== The most detailed description of the data in an SCLK file is provided in metadata included inside the description area of the file. This information can be viewed using any text editor program. Note that the SCLK kernels provided in this data set have been determined to be in a relativistic solar system barycentric frame of reference. This has been verified through confirmation that the ephemerides used to compute the SCLK kernel correlations are in a solar barycentric frame. It is critically important that the users of these kernels for time applications be aware of this and that they properly interpret the time correlations in the SCLK kernels. The file ``sea_2007_010.pdf'' in the ``document'' directory should be consulted for information on how to do this. In addition, the file ``sea_2003_024.pdf'' in the ``document'' directory gives further information on the format and design of these kernels. Contact Information =================== Regarding MESSENGER project specific information provided in this data set: Mike Reid (240)-228-4537 Mike.Reid@jhuapl.edu address: The Johns Hopkins University Applied Physics Laboratory 11100 Johns Hopkins Road Laurel, MD 20723 For general information about SPICE system: Charles H. Acton, Jr, (818)-354-3869, Charles.Acton@jpl.nasa.gov, or Boris Semenov (818)-354-8136 Boris.Semenov@jpl.nasa.gov address: Navigation and Ancillary Information Facility (NAIF) Jet Propulsion Laboratory MS 301-121 4800 Oak Grove Drive Pasadena CA 91109 USA