Phobos MRO/CRISM visible and near-infrared (0.5–2.5 μm) spectral modeling

This paper focuses on the spectral modeling of the surface of Phobos in the wavelength range between 0.5 and 2.5 μm. We exploit the Phobos Mars Reconnaissance Orbiter/Compact Reconnaissance Imaging Spectrometer for Mars (MRO/CRISM) dataset and extend the study area presented by Fraeman et al. (2012)...

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Bibliographic Details
Published in:Planetary and Space Science
Main Author: Marzo, G.A.
Other Authors: Marzo, G. A.
Format: Article in Journal/Newspaper
Language:English
Published: Elsevier Ltd 2018
Subjects:
Online Access:https://hdl.handle.net/20.500.12079/2013
https://doi.org/10.1016/j.pss.2018.02.016
https://www.scopus.com/inward/record.uri?eid=2-s2.0-85042922186&doi=10.1016%2fj.pss.2018.02.016&partnerID=40&md5=771b77722bee5024a751718b1be37ca0