urn:nasa:pds:magellan_bsr_calibrated:srf 1.0 1.22.0.0 Product_Collection 2025 The srf collection contains power spectra for the RCP and LCP channels which were used to 'equalize' (flatten) the spectral response of the filters in the receiving system. Since the filtering is entirely digital, there is no reason to believe that the RCP and LCP noise power spectra would differ; but separate srf files have been derived for the two channels. Standard deviation of individual frequency bins is about 1.3 percent of the mean. 2025-01-27 1.0 Initial version 1994-06-05T13:41:31Z 1994-06-05T13:48:11Z Science Calibrated Surface Geosciences Magellan Mission urn:nasa:pds:context:investigation:mission.magellan collection_to_investigation Alias: Venus Radar Mapper 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 collection_to_target BSR Calibration collection_srf_inventory.csv 2025-01-27 0 PDS DSV 1 2 Carriage-Return Line-Feed Comma 2 0 Member Status 1 ASCII_String 1 P indicates primary member of the collection S indicates secondary member of the collection LIDVID_LID 2 ASCII_LIDVID_LID 255 The LIDVID of a product that is a member of the collection. inventory_has_member_product