Effects of Palagonitic Dust Coatings on Visible, Near-IR, and Mössbauer Spectra of Rocks and Minerals: Implication for Mineralogical Remote Sensing of Mars

Details Effects of Palagonitic Dust Coatings on Visible, Near-IR, and Mössbauer Spectra of Rocks and Minerals: Implication for Mineralogical Remote Sensing of Mars Effects of Palagonitic Dust Coatings on Visible, Near-IR, and Mössbauer Spectra of Rocks and Minerals: Implication for Mineralogical Remote Sensing of Mars

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1912m&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1912

Physics

1

Scientific paper

Visible, near-IR, and Mossbauer measurements on dust coated rocks and
minerals show that a 300 µm thick layer is required to obscure the
substrate for VNIR measurements and that a >2000-µm-thick layer
is required to obscure the substrate for Mossbauer measurements.

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