Student or educator? Sign up with your school email and get 6 months of Pro free.
Cited by 1,114

The DOI matches its Crossref record; 107 of the 107 references it cites were found in a registry or an index.

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

Open access
Murchie, S., Arvidson, R., Bedini, P., Beisser, K., Bibring, J.‐P., Bishop, J., Boldt, J., Cavender, P., Choo, T., Clancy, R. T., Darlington, E. H., Des Marais, D., Espiritu, R., Fort, D., Green, R., Guinness, E., Hayes, J., Hash, C., Heffernan, K., Hemmler, J., Heyler, G., Humm, D., Hutcheson, J., Izenberg, N., Lee, R., Lees, J., Lohr, D., Malaret, E., Martin, T., McGovern, J. A., McGuire, P., Morris, R., Mustard, J., Pelkey, S., Rhodes, E., Robinson, M., Roush, T., Schaefer, E., Seagrave, G., Seelos, F., Silverglate, P., Slavney, S., Smith, M., Shyong, W.‐J., Strohbehn, K., Taylor, H., Thompson, P., Tossman, B., Wirzburger, M., Wolff, M.·2007·Journal of Geophysical Research: Planets

Abstract

The Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) is a hyperspectral imager on the Mars Reconnaissance Orbiter (MRO) spacecraft. CRISM consists of three subassemblies, a gimbaled Optical Sensor Unit (OSU), a Data Processing Unit (DPU), and the Gimbal Motor Electronics (GME). CRISM's objectives are (1) to map the entire surface using a subset of bands to characterize crustal mineralogy, (2) to map the mineralogy of key areas at high spectral and spatial resolution, and (3) to measure spatial and seasonal variations in the atmosphere. These objectives are addressed using three major types of observations. In multispectral mapping mode, with the OSU pointed at planet nadir, data are collected at a subset of 72 wavelengths covering key mineralogic absorptions and binned to pixel footprints of 100 or 200 m/pixel. Nearly the entire planet can be mapped in this fashion. In targeted mode the OSU is scanned to remove most along‐track motion, and a region of interest is mapped at full spatial and spectral resolution (15–19 m/pixel, 362–3920 nm at 6.55 nm/channel). Ten additional abbreviated, spatially binned images are taken before and after the main image, providing an emission phase function (EPF) of the site for atmospheric study and correction of surface spectra for atmospheric effects. In atmospheric mode, only the EPF is acquired. Global grids of the resulting lower data volume observations are taken repeatedly throughout the Martian year to measure seasonal variations in atmospheric properties. Raw, calibrated, and map‐projected data are delivered to the community with a spectral library to aid in interpretation.

Overview

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1029/2006je002682

Cites

107 of 107 references verified0 citation errors · 0 not checkable

Statistics

Verification

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Citations

Cites

Show all 107 references

Research works printed but not linked: 34

  1. 10.1346/CCMN.1994.0420511 · doi:10.1346/ccmn.1994.0420511
  2. Bishop J. L., 2002, Volcano‐Ice Interactions on Earth and Mars, 371
  3. Bishop J. L., 2003, The influence of glassy coatings on volcanic rocks from Mauna Iki, Hawaii and applications to rocks on Mars, Lunar Planet. Sci.
  4. Bugby D., 2005, Cryogenic Optical Systems and Instruments XI, 321
  5. Choo T. H., 2001, Workshop on Mercury: Space Environment, Surface, and Interior
  6. Christensen P. R., 1992, Mars, 686
  7. 10.1016/0019-1035(91)90169-T · doi:10.1016/0019-1035(91)90169-t
  8. Erard S., 1991, Spatial variations in composition of the Valles Marineris and Isidis Planitia regions of Mars derived for ISM spectra, Proc. Lunar Planet. Sci. Conf., 21, 437
  9. Farmer J., 1998, The Search for Life on Mars, 58
  10. Gíslason S., 1990, Fluid‐Mineral Interactions: A Tribute to H. P. Eugster, 373
  11. Hay R., 1977, Mineralogy and Geology of Natural Zeolites, 93, 10.1515/9781501508585-009 · doi:10.1515/9781501508585-009
  12. Jakosky B., 1992, Mars, 969
  13. Jouglet D., 2006, Observation of 3 μm hydration feature on Mars from OMEGA/Mars Express data, Lunar Planet. Sci.
  14. Kahn R., 1992, Mars, 1017
  15. Klingelhöfer G., 2005, MIMOS II on MER—One year of Mössbauer spectroscopy on the surface of Mars: From jarosite at Meridiani Planum to goethite at Gusev Crater, Lunar Planet. Sci., 2349
  16. Kraft D., 2003, Thermal emission spectra of silica‐coated basalt and considerations for Martian surface morphology, Lunar Planet. Sci.
  17. 10.1029/JB087iB08p06525 · doi:10.1029/jb087ib08p06525
  18. Lees J., 2005, Optomechanics 2005, 265
  19. Milliken R. E., 2006, The H2O content of the Martian surface as seen by Mars Express OMEGA, Lunar Planet. Sci.
  20. 10.1029/2001JE001518 · doi:10.1029/2001je001518
  21. Moroz V., 1964, The infrared spectrum of Mars (1.1–4.1 μm), Sov. Astron., 8, 273
  22. Morris R. V., 2003, Lunar Planet. Sci.
  23. Murchie S., 2004, Old desert varnish‐like coatings and young breccias at the Mars Pathfinder landing site, Lunar Planet. Sci.
  24. Mustard J., 2001, Unusual spectral properties observed in Valles Marineris, Lunar Planet. Sci., 2194
  25. Poulet F., 2005, Mineralogy of the northern high latitude regions of Mars, Lunar Planet. Sci., 1828
  26. 10.1029/2000JE001241 · doi:10.1029/2000je001241
  27. Schmitt B., 2005, Northern seasonal condensates on Mars by OMEGA/Mars Express, Lunar Planet. Sci., 2326
  28. 10.1007/BF00310959 · doi:10.1007/bf00310959
  29. 10.1117/12.504876 · doi:10.1117/12.504876
  30. Surdam R., 1977, Mineralogy and Geology of Natural Zeolites, 65, 10.1515/9781501508585-008 · doi:10.1515/9781501508585-008
  31. Troll J., 2005, Optomechanics 2005, 93
  32. Wang A., 2005, Sulfate deposition in regolith exposed in trenches on the plains between the Spirit landing site and Columbia Hills in Gusev Crater, Mars, Lunar Planet. Sci., 2236
  33. 10.1117/12.510204 · doi:10.1117/12.510204
  34. Zurek R., 1992, Mars, 835

Cited by

See all 1,114

Metadata

Authors
Murchie, S., Arvidson, R., Bedini, P., Beisser, K., Bibring, J. ‐., Bishop, J., Boldt, J., Cavender, P., Choo, T., Clancy, R. T., Darlington, E. H., Des Marais, D., Espiritu, R., Fort, D., Green, R., Guinness, E., Hayes, J., Hash, C., Heffernan, K., Hemmler, J., Heyler, G., Humm, D., Hutcheson, J., Izenberg, N., Lee, R., Lees, J., Lohr, D., Malaret, E., Martin, T., McGovern, J. A., McGuire, P., Morris, R., Mustard, J., Pelkey, S., Rhodes, E., Robinson, M., Roush, T., Schaefer, E., Seagrave, G., Seelos, F., Silverglate, P., Slavney, S., Smith, M., Shyong, W. ‐., Strohbehn, K., Taylor, H., Thompson, P., Tossman, B., Wirzburger, M., & Wolff, M.
Venue
Journal of Geophysical Research: Planets
Published
2007-05
Volume
112
Issue
E5
ISSN
0148-0227 (ISSN-L)
OpenAlex
W2126230369
Cited by
1,114
References
107
FWCI
30.40
Type
journal article
Language
en
Open access
bronze

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review

How to cite

Cite CoChat for the checks on this page, and the paper for its own findings.

This page
CoChat. (2026). Citation check: Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on Mars Reconnaissance Orbiter (MRO). https://app.cochat.ai/papers/10.1029/2006je002682
The paper
Murchie, S., Arvidson, R., Bedini, P., Beisser, K., Bibring, J. ‐., Bishop, J., Boldt, J., Cavender, P., Choo, T., Clancy, R. T., Darlington, E. H., Des Marais, D., Espiritu, R., Fort, D., Green, R., Guinness, E., Hayes, J., Hash, C., Heffernan, K., . . . Wolff, M. (2007). Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on Mars Reconnaissance Orbiter (MRO). Journal of Geophysical Research: Planets. https://doi.org/10.1029/2006je002682

Data sources

Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.