Mars Exploration Rover Athena Panoramic Camera (Pancam) investigation
By James F. Bell III, S. Squyres, K. Herkenhoff, J. Maki, H. Arneson, D. Brown, S. Collins, A. Dingizian, S. T. Elliot, E. Hagerott and 15 more. 2003
306 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Geology
View Paper: https://www.semanticscholar.org/paper/286c555a2f15561aa86e59ee2839aaab938aceac
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In Astronomy and Astrophysics
- Michael D. Smith
- Michael J. Wolff
- Mark T. Lemmon
- B. Cantor
- James F. Bell III
- S. Squyres
- Peter H. Smith
- Michael A. Caplinger
Citations in the corpus
- Eight-year climatology of dust optical depth on Mars (2014, unknown): “• PanCam cameras (Bell et al., 2003) aboard MER-A “Spirit” and MERB “Opportunity”, respectively from Ls ∼ 328◦ and Ls ∼ 339◦ in MY 26. Spirit PanCam stopped providing measurements after Ls ∼ 67◦ in MY 30. Lemmon et al. (2014) have retrieved CDOD from upward-”
- Spirit Mars Rover Mission: Overview and selected results from the northern Home Plate Winter Haven to the side of Scamander crater (2010, unknown): “This resistance can be modeled using classic Bekker‐Wong terramechanics theory [ Bekker, 1969; Wong, 2003].”
- The Mars Science Laboratory Curiosity rover Mastcam instruments: Preflight and in‐flight calibration, validation, and data archiving (2017, methodology): “…Mastcam coefficients in Table 4 for near-IR wavelengths greater than 800 nm that are comparable to the wavelengths used for the MER/Pancam filters [Bell et al., 2003] are essentially the same as those derived for the Pancams at room temperature, after compensating for differences in the focal…”
- Athena MIMOS II Mossbauer spectrometer investigation (2003, methodology): “Images and multispectral data obtained by Pancam [Bell et al., 2003] and Mini-TES [Christensen et al., 2003] complete full characterization of the target by the Athena instrument suite.”
- Dust aerosol, clouds, and the atmospheric optical depth record over 5 Mars years of the Mars Exploration Rover mission (2014, methodology): “calibration pipeline (Bell et al., 2006a), following the Bell et al. (2006a) flow from image input to flat-field removal.”