urn:nasa:pds:lp-mag-calibrated:data-lunarfield:98_306_03 1.0 1.20.0.0 Product_Observational Hood, Lon L. 2024 Lunar Prospector Magnetometer (MAG) Calibrated Data for 1998-11-02 Orbit: 03. Selected and filtered time series data at 5 second intervals from the Lunar Prospector (LP) polar orbital mission to the Moon (January 1998 to July 1999). 2025-03-19 1.0 This product, 98_306_03.TAB, was originally released as part of the PDS3 LP-L-MAG-4-LUNAR-FIELD-TS-V1.0 data set. The metadata have been migrated to PDS4. The data themselves are unchanged. 1998-11-02T09:11:02Z 1998-11-02T09:42:17Z Science Calibrated Lunar Prospector Calibrated MAG Data Fields Magnetic Background Lunar Prospector Mission urn:nasa:pds:context:investigation:mission.lunar_prospector data_to_investigation Lunar Prospector Host urn:nasa:pds:context:instrument_host:spacecraft.lp is_instrument_host Magnetometer Instrument urn:nasa:pds:context:instrument:lp.mag is_instrument Moon Satellite urn:nasa:pds:context:target:satellite.earth.moon data_to_target Primary Mission 03 03 urn:nasa:pds:lp-mager-derived:data-moon-pos:moon_pos::1.0 data_to_ancillary_data urn:nasa:pds:lp-mager-derived:data-spacecraft-pos:pos98_11::1.0 data_to_ancillary_data LP-L-MAG-4-LUNAR-FIELD-TS-V1.0:98_306_03:98_306_03.TAB data_to_calibrated_source_product 10.17189/1519723 PDS Planetary Plasma Interactions Node This is the first version converted to PDS4. The DOI references the source PDS3 data set. 98_306_03.TAB 2003-09-02T18:48:06 33464 adae479b7c7c19b76ac073089063e910 File naming convention: YY_DOY_NN.det, where YY is year number (98 or 99), DOY is day of year, and NN is orbit number on the selected day. Lunar Prospector Magnetic Field Vector Components for 1998-11-02 Orbit: 03 0 376 These data represent approximate measurements of the lunar crustal magnetic field with external (solar wind and magnetospheric) fields removed or minimized. Latitude / longitude coverage is limited to specific regions overpassed by the spacecraft during the selected intervals. Vector magnetic field components are given in two coordinate systems: Selenographic (SG) coordinates and east, north, and radial (ENR) coordinates. These data, archived after detrending, should only be used for studying crustal magnetic fields. The east, north, and radial version is the best one to use. If one needs to get the original magnetometer data including long-wavelength external fields as well as crustal fields, then one should go to a different data set (Level 1?). Note: The detrending of the data was done after the data were transformed into the various coordinate systems. As a result the values removed from the original time series data may differ slightly. Carriage-Return Line-Feed 10 0 89 Hour 1 1 ASCII_Real 9 Hour of the day in Universal time (to 4 decimal places). BE_ENR 2 11 ASCII_Real 7 nT East component of the magnetic field in ENR coordinates. BN_ENR 3 19 ASCII_Real 7 nT North component of the magnetic field in ENR coordinates. BR_ENR 4 27 ASCII_Real 7 nT Radial component of the magnetic field in ENR coordinates. Bx_SG 5 35 ASCII_Real 8 nT X component of the magnetic field in SG coordinates. By_SG 6 44 ASCII_Real 8 nT Y component of the magnetic field in SG coordinates. Bz_SG 7 53 ASCII_Real 8 nT Z component of the magnetic field in SG coordinates. Latitude 8 62 ASCII_Real 8 nT Lunar Latitude in degrees; north is positive. Longitude 9 71 ASCII_Real 8 nT Lunar east longitude in degrees. Altitude 10 80 ASCII_Real 8 km Approximate altitude of spacecraft in kilometers.