PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT INTERCHANGE_FORMAT = ASCII PUBLICATION_DATE = 2013-03-28 NOTE = "Cassini SP-Kernel Covariance Table Information" END_OBJECT = TEXT END Covariance Tables ================= This directory contains covariance table files describing the formal position uncertainties of Cassini's reconstructed ephemeris provided in the SPK files produced by the CASSINI NAV Team. These table files have the same names as the corresponding SPK files with an additional suffix set to the NAIF ID of the body with respect to which the uncertainties are given. All table file names have extension ``.txt''. For example, the table file ``060213R_SCPSE_05348_06005_606.txt'' describes the formal position uncertainties of Cassini's reconstructed ephemeris provided in the reconstructed SPK file ``060213R_SCPSE_05348_06005.bsp'' with respect to Titan (NAIF ID 606) as a function of time. Each covariance table file contains a single header record showing the field (column) names and one or more covariance matrix term data records, each comprising seven fields (columns). The first column labeled ``UTC'' contains the UTC time of the record. The columns labeled ``Rad'', ``Trans'', and ``Norm'' contain the covariance matrix diagonal terms, whereas the columns labeled ``Rad-Trans'', ``Rad-Norm'', and ``Trans-Norm'' list the covariance matrix off-diagonal terms. The ``Rad'' term is directed along the vector from body to Cassini, the ``Norm'' term is directed along the Cassini orbit angular momentum vector relative to body, and the ``Trans'' term is directed along the vector formed by ``Rad'' cross ``Norm''. Covariances can be assembled from the terms in each row (each time) as follows: Rad Rad-Trans Rad-Norm Rad-Trans Trans Trans-Norm Rad-Norm Trans-Norm Norm The square-root of each diagonal term is the one-sigma formal uncertainty along that direction. Dividing a non-diagonal term by the product of the square-roots of the diagonal terms in the corresponding row and column produces the correlation coefficient between the two directions. The covariance matrix terms represent formal one-sigma statistics. To account for possible systematic errors, scaling the uncertainties by a factor of three (scaling each row and each column of the covariance matrix by three) is advised in order to obtain a better portrayal of realistic uncertainties. Tables for some SPKs are missing and, if provided by the NAV team, will be added to the data set at a later time. A few tables have coverage shorter than the coverage of the corresponding SPK file. There is currently no plan to regenerate these tables to provide the complete coverage. Contact Information =================== Regarding Cassini project specific information provided in this data set and for general information about SPICE system: Boris Semenov (818)-354-8136 Boris.Semenov@jpl.nasa.gov address: Navigation and Ancillary Information Facility (NAIF) Jet Propulsion Laboratory MS 301-125L 4800 Oak Grove Drive Pasadena CA 91109 USA