PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM START_TIME = 1997-09-12T00:00:00 STOP_TIME = 1999-03-27T23:59:59 DATA_SET_ID = "MGS-M-RSS-5-SDP-V1.0" INSTRUMENT_HOST_NAME = "MARS GLOBAL SURVEYOR" TARGET_NAME = MARS PRODUCT_ID = "GGM0964B.PS1" ^PS_DOCUMENT = "GGM0964B.PS1" OBJECT = PS_DOCUMENT DOCUMENT_NAME = "WEST HEMISPHERE GRAVITY ANOMALIES FROM MGM0964C18" PUBLICATION_DATE = 1999-10-01 DOCUMENT_TOPIC_TYPE = "INITIAL EXPERIMENT RESULTS" INTERCHANGE_FORMAT = BINARY DOCUMENT_FORMAT = "POSTSCRIPT" FILES = 1 DESCRIPTION = " A PostScript rendition of gravity anomalies in file GGM0964A.IMG in the IMG directory of this archival volume. This file shows anomalies over 180-360E longitude and 60S to 60N latitude. Gravity anomalies are in milligals with respect to Mars gravity model MGM0964C18 evaluated to degree and order 50. The gravity anomalies are computed on a reference ellipsoid with the following constants: GM = 0.4282838041570575e+14 m**3/s**2, semi-major axis 3397000.0 m, 1991 IAU rotation rate (7.088218081252279e-4 rad/s), and inverse flattening for the ellipsoid (1/f) of 196.877360. Details of the analysis and results can be found in the DOCUMENT directory of this archival volume (see AAS99328.LBL). Or, see Lemoine et al., Paper AAS 99-328, Astrodynamics Specialist Conference, Girdwood, Alaska, 16-19 August 1999. This paper describes both MGM0964C18 and an improved model, MGM0964C20. See also Smith et al., 'The Gravity Field of Mars: Results from Mars Global Surveyor', Science, 286, 94-97, 1999. The PostScript file contains an unknown number of variable-length lines of ASCII characters. Lines are delimited by the ASCII carriage-return (ASCII 13) line-feed (ASCII 10) pair. This is a color PostScript file; but it has been successfully printed on a black and white printer. PostScript is a trademark of Adobe Systems, Inc." END_OBJECT = PS_DOCUMENT END