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Lunar UV-visible-IR mapping interferometric spectrometerUltraviolet-visible-infrared mapping digital array scanned interferometers for lunar compositional surveys was developed. The research has defined a no-moving-parts, low-weight and low-power, high-throughput, and electronically adaptable digital array scanned interferometer that achieves measurement objectives encompassing and improving upon all the requirements defined by the LEXSWIG for lunar mineralogical investigation. In addition, LUMIS provides a new, important, ultraviolet spectral mapping, high-spatial-resolution line scan camera, and multispectral camera capabilities. An instrument configuration optimized for spectral mapping and imaging of the lunar surface and provide spectral results in support of the instrument design are described.
Document ID
19930008076
Document Type
Conference Paper
Authors
Smith, W. Hayden (Washington Univ. Saint Louis, MO, United States)
Haskin, L. (Washington Univ. Saint Louis, MO, United States)
Korotev, R. (Washington Univ. Saint Louis, MO, United States)
Arvidson, R. (Washington Univ. Saint Louis, MO, United States)
Mckinnon, W. (Washington Univ. Saint Louis, MO, United States)
Hapke, B. (Pittsburgh Univ. PA., United States)
Larson, S. (Arizona Univ. Tucson., United States)
Lucey, P. (Hawaii Univ. Honolulu., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: Lunar and Planetary Inst., Joint Workshop on New Technologies for Lunar Resource Assessment
Subject Category
LUNAR AND PLANETARY EXPLORATION
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19930008044Analytic PrimaryJoint Workshop on New Technologies for Lunar Resource Assessment