urn:nasa:pds:magellan_gravity:gravity:geoid 1.0 1.20.0.0 Product_Observational Sjogren, William L. 1996 A digital map of Venus geoid derived from radio tracking of the Magellan spacecraft. 2023-09-06 1.0 Product migrated to PDS4 from PDS3. Magellan Mission urn:nasa:pds:context:investigation:mission.magellan data_to_investigation Magellan Host urn:nasa:pds:context:instrument_host:spacecraft.mgn is_instrument_host Radio Science Subsystem Instrument urn:nasa:pds:context:instrument:mgn.rss is_instrument Venus Planet urn:nasa:pds:context:target:planet.venus data_to_target SHXDR 5758 15019 JET PROPULSION LABORATORY Image_Object cartography_parameters_to_image_object -120.0 240.0 90.0 -90.0 Equirectangular 0 0 0 Coordinate Pair 105623.83567219283 105623.83567219283 1.0 1.0 -12674860.28066314 9506145.210497355 Planetocentric Venus (2015) - Sphere 6051800 6051800 6051800 Positive East Image_Object display_settings_to_array Sample Left to Right Line Top to Bottom geoid.dat 1996-05-31T12:00:00.000 This file contains a digital map of Venus geoid derived from radio tracking of the Magellan spacecraft. The observation is Venus geoid in meters at the surface referenced to a sphere of 6051.0 km radius. The map is produced by the Magellan Gravity Science Team at JPL under the direction of W.L. Sjogren.

0 5760 PDS3

Image_Object 5760 3 Last Index Fastest The Digital Map contains values of OBSERVATION_TYPE. The values can be obtained by multiplying the sample in the map by SCALING_FACTOR and then adding OFFSET. When BANDS is an even number, the even numbered maps (second, fourth, ..) will be the error maps (one-sigma uncertainty) for the immediately preceding odd-numbered maps (first, third, ...). The uncertainty value can be obtained by multiplying the sample in the error map by SCALING_FACTOR; the OFFSET is not used in these cases. OBSERVATION_TYPE = 'GEOID IN METERS' IEEE754MSBDouble meter 1.0 0.0 Band 2 1 Line 180 2 Sample 360 3