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- W4306148344 abstract "Thermal infrared instruments have proven integral components on payloads across the solar system, including the highlights below. The Voyager payload included the IRIS spectrometer [1] that provided our first views of the thermal emission spectra of several satellites, as well as the thermal emission and global heat balance of the four giant planets [1] . The Galileo payload included the Photopolarimeter-Radiometer PPR experiment that provided new constraints on the heat flow from Io and an upper limit on Europa [2] . The Cassini payload included the Composite Infrared Spectrometer (CIRS) that provided thermal and composition mapping of Saturn’s atmosphere and satellites, including Titan [3] and anomalous thermal emission due to active endogenic heat sources on Enceladus [4] . Mars remains a popular target for thermal infrared instruments dating back to the Infrared Thermal Mapper (IRTM) on the Viking orbiters, through the Mars Global Surveyor Thermal Emission Spectrometer (TES) to the current flight instruments: Thermal Emission Imaging System (THEMIS) on Mars Odyssey and MCS on MRO [5] , [6] . MCS is an atmospheric limb sounder that measures 4-D global fields of temperature, pressure, dust, and ices in the atmosphere of Mars, both day and night. Diviner on LRO [10] is providing a complete set of precise radiometric lunar surface temperature measurements over its full 30-400 K range, as well as constraints on physical and compositional properties." @default.
- W4306148344 created "2022-10-14" @default.
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- W4306148344 date "2022-09-01" @default.
- W4306148344 modified "2023-09-30" @default.
- W4306148344 title "Uncooled Infrared/Far-Infrared Thermopile Arrays for Space-Borne, Remote-Sensing Radiometry" @default.
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- W4306148344 doi "https://doi.org/10.1109/rapid54472.2022.9911570" @default.
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