urn:nasa:pds:clementine1_bistatic:calib:df2scm 1.0 1.21.0.0 Product_Observational 1999 Coefficients for piecewise linear prediction of frequency of South Pole bin in receiver baseband output. Assumes Clementine S-band carrier signal is fixed at 12500 Hz. Table gives constant and linear terms for time segments of (usually) one second from 67001 to 67969 seconds on 9 April 1994 as seen at DSS 14. Predictions were computed using Stanford program DF2SCM and results from earlier calculations in programs BSRGEOM and BSRDOP. To find frequency F of South Pole bin at time T, find the row for which T0 <= T < T1 and compute F = F0 + DFDT*(T-T0). 2024-04-23 1.0 Product migrated to PDS4 from PDS3. Deep Space Program Science Experiment Mission urn:nasa:pds:context:investigation:mission.deep_space_program_science_experiment data_to_investigation Clementine 1 Clementine 1 Host urn:nasa:pds:context:instrument_host:spacecraft.clem1 is_instrument_host Radio Science Subsystem Instrument urn:nasa:pds:context:instrument:clem1.rss is_instrument Moon Satellite urn:nasa:pds:context:target:satellite.earth.moon data_to_target df2scm.tab SOUTH POLE FREQUENCY 0 968 Table has 4 columns, 968 rows. Values are ASCII real numbers, delimited by commas. First two columns require 23 bytes; third column uses 13, and last column uses 12. Rows are delimited by an ASCII carriage-return (ASCII 13) line-feed pair (ASCII 10), making 76 bytes per row. Carriage-Return Line-Feed 4 0 76 F0 1 1 ASCII_Real 23 hertz Frequency of the South Pole bin at the beginning of this time interval DFDT 2 25 ASCII_Real 23 hertz per second Rate at which the frequency of the South Pole bin changes during this time interval T0 3 49 ASCII_Real 13 second Earth receive time (UTC) in seconds at the beginning of this time interval T1 4 63 ASCII_Real 12 second Earth receive time (UTC) in seconds at the end of this time interval df2scm.lbl 0 PDS3 Original PDS3 label Carriage-Return Line-Feed