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AGU: Journal of Geophysical Research, Planets

 

Keywords

  • Mars Exploration Rovers
  • Navcam
  • instrument calibration

Index Terms

  • Planetary Sciences: Solar System Objects: Mars
  • Planetary Sciences: Solar System Objects: Instruments and techniques
  • Planetary Sciences: Solid Surface Planets: Remote sensing
  • Planetary Sciences: Solid Surface Planets: Surface materials and properties
  • Planetary Sciences: Solid Surface Planets: Instruments and techniques
Abstract
Cited By (0)
 

Abstract

Mars Exploration Rover Navigation Camera in-flight calibration

Jason M. Soderblom

Department of Astronomy, Cornell University, Ithaca, New York, USA

Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona, USA

James F. Bell III

Department of Astronomy, Cornell University, Ithaca, New York, USA

Jeffrey R. Johnson

Astrogeology Team, U.S. Geological Survey, Flagstaff, Arizona, USA

Jonathan Joseph

Department of Astronomy, Cornell University, Ithaca, New York, USA

Michael J. Wolff

Space Science Institute, Boulder, Colorado, USA

The Navigation Camera (Navcam) instruments on the Mars Exploration Rover (MER) spacecraft provide support for both tactical operations as well as scientific observations where color information is not necessary: large-scale morphology, atmospheric monitoring including cloud observations and dust devil movies, and context imaging for both the thermal emission spectrometer and the in situ instruments on the Instrument Deployment Device. The Navcams are a panchromatic stereoscopic imaging system built using identical charge-coupled device (CCD) detectors and nearly identical electronics boards as the other cameras on the MER spacecraft. Previous calibration efforts were primarily focused on providing a detailed geometric calibration in line with the principal function of the Navcams, to provide data for the MER navigation team. This paper provides a detailed description of a new Navcam calibration pipeline developed to provide an absolute radiometric calibration that we estimate to have an absolute accuracy of 10% and a relative precision of 2.5%. Our calibration pipeline includes steps to model and remove the bias offset, the dark current charge that accumulates in both the active and readout regions of the CCD, and the shutter smear. It also corrects pixel-to-pixel responsivity variations using flat-field images, and converts from raw instrument-corrected digital number values per second to units of radiance (W m−2 nm−1 sr−1), or to radiance factor (I/F). We also describe here the initial results of two applications where radiance-calibrated Navcam data provide unique information for surface photometric and atmospheric aerosol studies.

Received 6 September 2007; accepted 24 April 2008; published 17 June 2008.

Citation: Soderblom, J. M., J. F. Bell III, J. R. Johnson, J. Joseph, and M. J. Wolff (2008), Mars Exploration Rover Navigation Camera in-flight calibration, J. Geophys. Res., 113, E06S19, doi:10.1029/2007JE003003.

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