The Mars Science Laboratory Curiosity rover Mastcam instruments: Preflight and in‐flight calibration, validation, and data archiving
By Jimmy D Bell, A. Godber, S. McNair, Michael A. Caplinger, J. Maki, Mark T. Lemmon, J. Beek, Michael C. Malin, D. Wellington, K. Kinch and 10 more. 2017
148 citations recorded by the source corpus.
The NASA Curiosity rover Mast Camera (Mastcam) system is a pair of fixed‐focal length, multispectral, color CCD imagers mounted ~2 m above the surface on the rover's remote sensing mast, along with associated electronics and an onboard calibration target. The left Mastcam (M‐34) has a 34 mm focal length, an instantaneous field of view (IFOV) of 0.22 mrad, and a FOV of 20° × 15° over the full 1648 × 1200 pixel span of its Kodak KAI‐2020 CCD. The right Mastcam (M‐100) has a 100 mm focal length, an IFOV of 0.074 mrad, and a FOV of 6.8° × 5.1° using the same detector. The cameras are separated by 24.2 cm on the mast, allowing stereo images to be obtained at the resolution of the M‐34 camera. Each camera has an eight‐position filter wheel, enabling it to take Bayer pattern red, green, and blue (RGB) “true color” images, multispectral images in nine additional bands spanning ~400–1100 nm, and images of the Sun in two colors through neutral density‐coated filters. An associated Digital Electronics Assembly provides command and data interfaces to the rover, 8 Gb of image storage per camera, 11 bit to 8 bit companding, JPEG compression, and acquisition of high‐definition video. Here we describe the preflight and in‐flight calibration of Mastcam images, the ways that they are being archived in the NASA Planetary Data System, and the ways that calibration refinements are being developed as the investigation progresses on Mars. We also provide some examples of data sets and analyses that help to validate the accuracy and precision of the calibration.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/86d42153920a3ee3dfc344edb1fb26ee76d75fcb
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In Astronomy and Astrophysics
- James F. Bell III
- John P. Grotzinger
- Ashwin R. Vasavada
- K. Edgett
- James W. Head III
- A. S. McEwen
- Ralph E. Milliken
- Nicolas Gonzalez Thomas
Citations in the corpus
- Ancient Martian aeolian processes and palaeomorphology reconstructed from the Stimson formation on the lower slope of Aeolis Mons, Gale crater, Mars (2018, methodology): “Coverage obtained by the Mastcams limited by data volumes that can be stored onboard (8 Gb per camera) (Bell et al., 2017) and bandwidth limitations associated with interplanetary communications.”