Reflectance spectra of selected lunar areas within the 300 - 800 nm spectral range observed by means of the SVET instrument and their interpretation.

Details Reflectance spectra of selected lunar areas within the 300 - 800 nm spectral range observed by means of the SVET instrument and their interpretation. Reflectance spectra of selected lunar areas within the 300 - 800 nm spectral range observed by means of the SVET instrument and their interpretation.

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994avest..28...49k&link_type=abstract

Astronomicheskii Vestnik, Tom 28, No. 6, p. 49 - 69

Astronomy and Astrophysics

Astronomy

Moon Surface: Regolith, Moon Surface: Reflectance Spectra, Moon Surface: Mineralogy

Scientific paper

The SVET instrument has been designed and built for use of Mars mineralogy mapping. Placed at the 2-m telescope at the high altitude Pic-du-Midi observatory and observing the Moon. The observations provide two kinds of results. Firstly, the validity of the design was proved, secondly - some interesting results on spectral characteristics and content of lunar regolith were obtained.

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