urn:nasa:pds:a15_17_hfe_concatenated:data:a17_1977p2f1_clean 1.0 1.12.0.0 Product_Observational St. Clair, M; Million, C.; Siegler, M. Ward, J. 2019 This table contains data from parts of 1977 for the upper gradient bridge of Apollo 17 probe 2 in this bundle's 'clean' format. This format flags impulsive outliers and missing data using a bitmask, adds a corrected dT range to some Lamont-NSSDC data, reorders some inverted time points, and places data from Nagihara et al. into the format of the Lamont-NSSDC data. See bundle_documentation.md for details. It is basically a converted, reformatted, and marked-up version of data released by Nagihara et al. along with "Examination of the Long‐Term Subsurface Warming Observed at the Apollo 15 and 17 Sites Utilizing the Newly Restored Heat Flow Experiment Data From 1975 to 1977," JGR Planets 123 (5), May 2018, doi: 10.1029/2018JE005579. 2020-02-13 1.0 Initial version. 1977-04-25T06:33:34.590Z 1977-09-30T18:06:22.080Z Apollo 17 Mission urn:nasa:pds:context:investigation:mission.apollo_17 data_to_investigation APOLLO 17 LUNAR SURFACE EXPERIMENTS PACKAGE Spacecraft urn:nasa:pds:context:instrument_host:spacecraft.a17a is_instrument_host HEAT FLOW EXPERIMENT Instrument urn:nasa:pds:context:instrument:hfe.a17a is_instrument Moon Satellite urn:nasa:pds:context:target:satellite.earth.moon data_to_target 10.1029/2018JE005579 data_to_derived_source_product 10.1029/2018JE005579 Data released with publication: Nagihara et al., Examination of the Long‐Term Subsurface Warming Observed at the Apollo 15 and 17 Sites Utilizing the Newly Restored Heat Flow Experiment Data From 1975 to 1977, JGR Planets 123 (5), May 2018. Contains data recovered from ARCSAV tapes. a17_1977p2f1.tab 1850883 28920

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a17_1977p2f1 68 28919 This table contains data from parts of 1977 for the upper gradient bridge of Apollo 17 probe 2 in this bundle's 'clean' format. This format flags impulsive outliers and missing data using a bitmask, adds a corrected dT range to some Lamont-NSSDC data, reorders some inverted time points, and places data from Nagihara et al. into the format of the Lamont-NSSDC data. See bundle_documentation.md for details. It is basically a converted, reformatted, and marked-up version of data released by Nagihara et al. along with "Examination of the Long‐Term Subsurface Warming Observed at the Apollo 15 and 17 Sites Utilizing the Newly Restored Heat Flow Experiment Data From 1975 to 1977," JGR Planets 123 (5), May 2018, doi: 10.1029/2018JE005579 Carriage-Return Line-Feed 4 0 64 Time 1 1 ASCII_Real 17 ms Earth-received time expressed in the 'mission epoch' format used by the original investigators: total ms from midnight on December 31, 1971. T 2 19 ASCII_Real 14 K Average temperature of the bridge's thermometers. Nagihara et al. give explicit temperatures for each thermometer. We compute T by simply averaging these values. dT 3 34 ASCII_Real 14 K Temperature difference between the lower and upper thermometers of the bridge. Positive values mean the lower thermometer is warmer. Nagihara et al. give explicit temperatures for each thermometer. We compute dT by simply taking the difference of these values. flags 4 49 ASCII_Real 14 Bitmask marking special features of some data points. See bundle_documentation.md for details.