| タイトル | The Moon Mineralogy (M3) Imaging Spectrometer: Early Assessment of the Spectral, Radiometric, Spatial and Uniformity Properties |
| 本文（外部サイト） | http://hdl.handle.net/2060/20090025993 |
| 著者（英） | Eastwood, M.; Plourde, K.; Rodriquez, J.; Bruce, C.; Boardman, J.; Haemmerle, V.; Glavich, T.; Koch, T.; Green, Robert O.; Racho, C.; Paulson, S.; Lundeen, S.; Hovland, L.; Bousman, J.; Green, R.; Chatterjee, A.; Geier, S.; Motts, E.; Barr, D.; Lee, K.; Pieters, C. M.; Hyman, S.; Robinson, D.; Essandoh, V.; Mouroulis, P. |
| 著者所属（英） | Jet Propulsion Lab., California Inst. of Tech. |
| 発行日 | 2009-01-29 |
| 言語 | eng |
| 内容記述 | The Moon Mineralogy Mapper's (M3) is a high uniformity and high signal-to-noise ratio NASA imaging spectrometer that is a guest instrument on the Indian Chandrayaan-1 Mission to the Moon. The laboratory measured spectral, radiometric, spatial, and uniformity characteristics of the M3 instrument are given. The M3 imaging spectrometer takes advantage of a suite of critical enabling capabilities to achieve its measurement requirement with a mass of 8 kg, power usage of 15 W, and volume of 25X18X12 cm. The M3 detector and spectrometer are cooled by a multi-stage passive cooler. This paper presents early M3 performance assessment results. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| レポートNO | MSFC-2216 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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