Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on Mars Reconnaissance Orbiter (MRO)

By Scott L. Murchie, R. Arvidson, P. Bedini, K. Beisser, J. Bibring, Janice L. Bishop, J. Boldt, P. Cavender, T. Choo, R. Clancy and 40 more. 2007

1,065 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Astronomy and Astrophysics, Ecology

View Paper: https://www.semanticscholar.org/paper/3e462253c251aae468193b6b66cf4b0dc60698ca

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Citations in the corpus

Mineralogy of the Martian Surface (2014, background): “…et al. 2005 2006–present CRISM Compact Reconnaissance Imaging Spectrometer for Mars Orbit Visible/near-infrared imaging spectroscopy (0.4–4.0 μm; 18–200 m/pixel) Murchie et al. 2007 2004–2011 (Spirit) 2004–present (Opportunity) MB Mössbauer Spectrometer Rover Arm-based in situ…”
The High Resolution Imaging Science Experiment (HiRISE) during MRO’s Primary Science Phase (PSP) (2010, methodology): “…database at JPL, then produce and validate the products to be shared with users (the HiRISE science team, other MRO investigators, the Mars Exploration Program, the Mars science community, and the general public), ultimately delivering archived products to the NASA Planetary Data System (PDS).”
Reflectance and emission spectroscopy study of four groups of phyllosilicates: smectites, kaolinite-serpentines, chlorites and micas (2008, methodology): “We focused on the visible/near-infrared (VNIR) region from 0.4 4.0 mm measured by Mars Express/OMEGA (Bibring et al., 2005), MRO/CRISM (Murchie et al., 2007) and partially covered by Mars Exploration Rover/Pancam (Bell et al., 2006), as well as the midIR region (5 50 mm) covered by MGS/TES…”
Revised CRISM spectral parameters and summary products based on the currently detected mineral diversity on Mars (2014, background): “Iron oxides have been detected through telescopic, orbital, and in situ observations of the surface of Mars, through the strong ferric absorption edge at 0.53μm [Bell et al., 1992; Morris et al., 2000; Farrand et al., 2006; Poulet et al., 2007].”
The Polar Deposits of Mars (2009, methodology): “Mars Reconnaissance Orbiter (MRO) CRISM Compact Reconnaissance Imaging Spectrometer for Mars (Murchie et al. 2007a) HiRISE High Resolution Imaging Science Experiment (McEwen et al. 2007) SHARAD Mars Shallow Subsurface Radar (Seu et al. 2007b) Mars Express (MEX) MARSIS Mars Advanced Radar for…”
Water and Brines on Mars: Current Evidence and Implications for MSL (2013, background): “MRO’s Compact Reconnaissance Imaging Spectrometer (CRISM) (Murchie et al. 2007) has not identified specific absorption features expected from liquid water in RSL.”
An improvement to the volcano-scan algorithm for atmospheric correction of CRISM and OMEGA spectral data (2009, methodology): “See Murchie et al. (2007) for a description of the multispectral mode of CRISM; CRISM “multispectral data” is used for survey observation and, for data volume management reasons, includes a subset of the spectral channels of the full hyperspectral images.”
The High Resolution Stereo Camera (HRSC) of Mars Express and its approach to science analysis and mapping for Mars and its satellites (2016, background): “…and spectroscopic data sets from instruments providing global coverage for Mars such as the Observatoire pour la Minéralogie, l’Eau, les Glaces et l’Activité of Mars Express (OMEGA, Bibring et al., 2006) or the Compact Reconnaissance Imaging Spectrometer for Mars of MRO (CRISM; Murchie, 2007).”
A synthesis of Martian aqueous mineralogy after 1 Mars year of observations from the Mars Reconnaissance Orbiter (2009, background): “Citation: Murchie, S. L., et al. (2009), A synthesis of Martian aqueous mineralogy after 1 Mars year of observations from the Mars”
Compact Reconnaissance Imaging Spectrometer for Mars investigation and data set from the Mars Reconnaissance Orbiter's primary science phase (2009, methodology): “Introduction [2] The Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) [Murchie et al., 2007a] is one of six major science instruments on the Mars Reconnaissance Orbiter (MRO), along with the High Resolution Imaging Science Experiment (HiRISE) [McEwen et al., 2007], the Mars Color Imager…”