Derivation of the VNIR (0.4-4.0 µm) Optical Constants of Nontronite and an Application to Mars: Modeling Single Scattering Albedo of Candidate Martian Dust Grains

Details Derivation of the VNIR (0.4-4.0 µm) Optical Constants of Nontronite and an Application to Mars: Modeling Single Scattering Albedo of Candidate Martian Dust Grains Derivation of the VNIR (0.4-4.0 µm) Optical Constants of Nontronite and an Application to Mars: Modeling Single Scattering Albedo of Candidate Martian Dust Grains

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2436r&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Computer Science

Scientific paper

We derive optical constants of nontronite using two scattering theories.
Mie scattering models compare palagonite and nontronite as putative
martian atmospheric dust and show the importance of knowing these
optical contants for quantitative interpretation of CRISM spectra.

Affiliated with

Also associated with

No associations

Rating

Derivation of the VNIR (0.4-4.0 µm) Optical Constants of Nontronite and an Application to Mars: Modeling Single Scattering Albedo of Candidate Martian Dust Grains does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Derivation of the VNIR (0.4-4.0 µm) Optical Constants of Nontronite and an Application to Mars: Modeling Single Scattering Albedo of Candidate Martian Dust Grains, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Derivation of the VNIR (0.4-4.0 µm) Optical Constants of Nontronite and an Application to Mars: Modeling Single Scattering Albedo of Candidate Martian Dust Grains will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-775284