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ChemCam passive reflectance spectroscopy of surface materials at the Curiosity landing site, Mars
Johns Hopkins University Applied Physics Laboratory, Laurel.
Arizona State University.
Planetary Science Institute, Tucson.
Jet Propulsion Laboratory, Pasadena, Kalifornien.
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2015 (English)In: Icarus (New York, N.Y. 1962), ISSN 0019-1035, E-ISSN 1090-2643, Vol. 249, p. 74-92Article in journal (Refereed) Published
Abstract [en]

The spectrometers on the Mars Science Laboratory (MSL) ChemCam instrument were used in passive mode to record visible/near-infrared (400–840 nm) radiance from the martian surface. Using the onboard ChemCam calibration targets’ housing as a reflectance standard, we developed methods to collect, calibrate, and reduce radiance observations to relative reflectance. Such measurements accurately reproduce the known reflectance spectra of other calibration targets on the rover, and represent the highest spatial resolution (0.65 mrad) and spectral sampling (

Place, publisher, year, edition, pages
2015. Vol. 249, p. 74-92
National Category
Aerospace Engineering
Research subject
Atmospheric science
Identifiers
URN: urn:nbn:se:ltu:diva-2717DOI: 10.1016/j.icarus.2014.02.028Scopus ID: 2-s2.0-85028160231Local ID: 0659e994-13b9-45ad-8f9c-9826d15395c5OAI: oai:DiVA.org:ltu-2717DiVA, id: diva2:975570
Note

Godkänd; 2015; Bibliografisk uppgift: Javier Martin-Torres ingår i MSL Science Team; 20150330 (ninhul)

Available from: 2016-09-29 Created: 2016-09-29 Last updated: 2018-08-16Bibliographically approved

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