urn:nasa:pds:clementine_lwir_bt:miscellaneous:calindex 1.0 1.17.0.0 Product_Ancillary 2023-10-25 1.0 Data migrated to PDS4 1994-02-27T07:04:02.174Z 1994-04-22T23:08:09.091Z DEEP SPACE PROGRAM SCIENCE EXPERIMENT Mission urn:nasa:pds:context:investigation:mission.deep_space_program_science_experiment ancillary_to_investigation CLEMENTINE 1 Host urn:nasa:pds:context:instrument_host:spacecraft.clem1 is_instrument_host LONG WAVELENGTH INFRARED CAMERA Instrument urn:nasa:pds:context:instrument:lwir.clem1 is_instrument Moon Satellite urn:nasa:pds:context:target:satellite.earth.moon ancillary_to_target calindex.tab 0 PDS DSV 1 This index table contains parameters that describe the flat field and bad pixel images from the Clementine LWIR brightness temperature dataset. 1362 Carriage-Return Line-Feed Comma 8 0 PDS3_volume_ID 1 ASCII_String The PDS3 volume_id element provides a unique identifier for a data volume. file_specification_name 2 ASCII_String Path and file name for the image file. product_id 3 ASCII_String The pds3 product_id data element represents a unique identifier assigned to a data product. product_type 4 ASCII_String The product type data element identifies the type or category of a data product within a data set. mission_phase_name 5 ASCII_String The mission_phase_name element provides the commonly-used identifier of a mission phase. target_name 6 ASCII_String Observed target. revolution_number 7 ASCII_Integer The revolution number refers to an observational pass over the moon. Revolution number is incremented by one each time the spacecraft passes over the south pole prior to the beginning of data acquisition. It is used in lieu of orbit number because is incremented at the equator on the sunlit side of the Moon. Thus, orbit number is changed in the middle of an observational pass. This was awkward in defining data acquired by a single pass over the Moon. product_creation_time 8 ASCII_Date_Time_YMD The time that the data file was created.