Vis/nir Spectral Differences of Materials within Gale Crater, Mars: Parameterization of Msl/mastcam Multispectral Observations
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Jim Bell 1 1 JAMES F . BELL III : PUBLICATIONS AS OF OCTOBER 2017 FIRST AUTHORED PEER
S AND CONFERENCE PRESENTATIONS 622. Kwan, C., B. Budavari, M. Dao, B. Ayhan J.F. Bell III, Pansharpening of Mastcam Images, IEEE International Geoscience and Remote Sensing Symposium, July 23–28, Fort Worth, Texas, 2017. 621. Dao, M., C. Kwan, A. Bulent, and J.F. Bell III, Enhancing Mastcam Images for Mars Rover Mission, 14th International Symposium on Neural Networks (ISNN 2017), Sapporo, Hokk...
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Background: Gale Crater is located at 5.3°S, 222.3°W (137.7°E) and has a diameter of ~155 km. It has b een a ta rget o f p articular i nterest d ue to the > 5 k m t all m ound o f layered material that occupies the center of the c rater. Gale Crater is currently one of four finalist landing s ites for the Mars Science Laboratory rover. Method: We used visible (CTX, HiRISE, MOC), infrared (THEMI...
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