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Found 495 dataset(s) matching "lunar".
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This dataset contains calibrated, 1.05- to 4.8-micron spectral images of comet 9P/Tempel 1 the acquired by the High Resolution Infrared Spectrometer (HRII) from 20 June through 06 July 2005 during...
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The Airborne Visible and Infared Imaging Spectrometer (AVIRIS) data are divided into 10x10 square kilometer scenes for purposes of standard product generation. More than 40 scenes were generated...
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The Airborne Visible and Infared Imaging Spectrometer (AVIRIS) data are divided into 10x10 square kilometer scenes for purposes of standard product generation. More than 40 scenes were generated...
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PARABOLA data were obtained at three GRSFE modeling sites in the Lunar Crater Volcanic Field. The playa site, the cobble site, and the mantled flow site. Each site was imaged by PARABOLA at a...
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PARABOLA data were obtained at three GRSFE modeling sites in the Lunar Crater Volcanic Field. The playa site, the cobble site, and the mantled flow site. Each site was imaged by PARABOLA at a...
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This data set consists of optical depth measurements made using the the Reagan Radiometer (acquired data in July 17 and September 29, 1989 at Lunar Lake). Total instantaneous optical depth was...
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This data set consists of optical depth measurements made using the the Reagan Radiometer (acquired data in July 17 and September 29, 1989 at Lunar Lake). Total instantaneous optical depth was...
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Spectral hygrometer (SHYG) data were gathered on September 29, 1989 at Lunar Lake. The spectral hygrometer provided the ratio Rsh=L(935)/L(880), where L(935) is the radiance at 935 nm. The...
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Spectral hygrometer (SHYG) data were gathered on September 29, 1989 at Lunar Lake. The spectral hygrometer provided the ratio Rsh=L(935)/L(880), where L(935) is the radiance at 935 nm. The...
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The SIRIS measurement objectives were: 1) to measure reflectance spectra of a bright and dark target at each GRSFE site for potential use in AVIRIS calibration characterize selected sites at the...
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The SIRIS measurement objectives were: 1) to measure reflectance spectra of a bright and dark target at each GRSFE site for potential use in AVIRIS calibration characterize selected sites at the...
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The weather station (WTHS) data consist of wind velocity, direction, and air temperature collected at Lunar Lake during the July and September field campaigns. Data were digitized at 30 minute...
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The weather station (WTHS) data consist of wind velocity, direction, and air temperature collected at Lunar Lake during the July and September field campaigns. Data were digitized at 30 minute...
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This data set contains archival raw science data, acquired from the Lunar Gravity Ranging System (LGRS) on each of the two spacecraft comprising the Gravity Recovery and Interior Laboratory...
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This data set contains archival raw science data, acquired from the Lunar Gravity Ranging System (LGRS) on each of the two spacecraft comprising the Gravity Recovery and Interior Laboratory...
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This data set contains calibrated and resampled engineering (e.g., star tracker data and timing) and science data acquired from the Lunar Gravity and Ranging System (LGRS) on the two spacecraft...
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This data set contains calibrated and resampled engineering (e.g., star tracker data and timing) and science data acquired from the Lunar Gravity and Ranging System (LGRS) on the two spacecraft...
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This data set contains archival derived science data, acquired from the Lunar Gravity Ranging System (LGRS) on the two spacecraft comprising the Gravity Recovery and Interior Laboratory (GRAIL)...
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This data set contains archival derived science data, acquired from the Lunar Gravity Ranging System (LGRS) on the two spacecraft comprising the Gravity Recovery and Interior Laboratory (GRAIL)...
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This data set consists of a series of images of the Moon showing radar scaled echo power. Each covers about 400 square kilometers of the lunar surface, and contains two co-registered images....
