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The Mars Science Laboratory (MSL) Mast cameras and Descent imager: Investigation and instrument descriptions.
Malin, Michal C; Ravine, Michael A; Caplinger, Michael A; Tony Ghaemi, F; Schaffner, Jacob A; Maki, Justin N; Bell, James F; Cameron, James F; Dietrich, William E; Edgett, Kenneth S; Edwards, Laurence J; Garvin, James B; Hallet, Bernard; Herkenhoff, Kenneth E; Heydari, Ezat; Kah, Linda C; Lemmon, Mark T; Minitti, Michelle E; Olson, Timothy S; Parker, Timothy J; Rowland, Scott K; Schieber, Juergen; Sletten, Ron; Sullivan, Robert J; Sumner, Dawn Y; Aileen Yingst, R; Duston, Brian M; McNair, Sean; Jensen, Elsa H.
Afiliação
  • Malin MC; Malin Space Science Systems, Inc San Diego California USA.
  • Ravine MA; Malin Space Science Systems, Inc San Diego California USA.
  • Caplinger MA; Malin Space Science Systems, Inc San Diego California USA.
  • Tony Ghaemi F; Ghaemi Optical Engineering San Diego California USA.
  • Schaffner JA; Malin Space Science Systems, Inc San Diego California USA.
  • Maki JN; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA.
  • Bell JF; School of Earth and Space Exploration Arizona State University Tempe Arizona USA.
  • Cameron JF; Lightstorm Entertainment Manhattan Beach California USA.
  • Dietrich WE; Department of Earth and Planetary Science University of California Berkeley California USA.
  • Edgett KS; Malin Space Science Systems, Inc San Diego California USA.
  • Edwards LJ; NASA Ames Research Center Moffett Field California USA.
  • Garvin JB; NASA Goddard Space Flight Center Greenbelt Maryland USA.
  • Hallet B; Department of Earth and Space Sciences, College of the Environment University of Washington Seattle Washington USA.
  • Herkenhoff KE; U.S. Geological Survey Flagstaff Arizona USA.
  • Heydari E; Department of Physics, Atmospheric Sciences, and Geoscience Jackson State University Jackson Mississippi USA.
  • Kah LC; Department of Earth and Planetary Sciences University of Tennessee, Knoxville Knoxville Tennessee USA.
  • Lemmon MT; Department of Atmospheric Sciences Texas A&M University College Station Texas USA.
  • Minitti ME; Planetary Science Institute Tucson Arizona USA.
  • Olson TS; Salish Kootenai College Pablo Montana USA.
  • Parker TJ; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA.
  • Rowland SK; Department of Geology and Geophysics, School of Ocean and Earth Science and Technology University of Hawai'i at Manoa Honolulu HI USA.
  • Schieber J; Department of Earth and Atmospheric Sciences Indiana University, Bloomington Bloomington Indiana USA.
  • Sletten R; Department of Earth and Space Sciences, College of the Environment University of Washington Seattle Washington USA.
  • Sullivan RJ; Department of Astronomy Cornell University Ithaca New York USA.
  • Sumner DY; Department of Earth and Planetary Sciences University of California Davis California USA.
  • Aileen Yingst R; Planetary Science Institute Tucson Arizona USA.
  • Duston BM; Malin Space Science Systems, Inc San Diego California USA.
  • McNair S; Malin Space Science Systems, Inc San Diego California USA.
  • Jensen EH; Malin Space Science Systems, Inc San Diego California USA.
Earth Space Sci ; 4(8): 506-539, 2017 08.
Article em En | MEDLINE | ID: mdl-29098171
ABSTRACT
The Mars Science Laboratory Mast camera and Descent Imager investigations were designed, built, and operated by Malin Space Science Systems of San Diego, CA. They share common electronics and focal plane designs but have different optics. There are two Mastcams of dissimilar focal length. The Mastcam-34 has an f/8, 34 mm focal length lens, and the M-100 an f/10, 100 mm focal length lens. The M-34 field of view is about 20° × 15° with an instantaneous field of view (IFOV) of 218 µrad; the M-100 field of view (FOV) is 6.8° × 5.1° with an IFOV of 74 µrad. The M-34 can focus from 0.5 m to infinity, and the M-100 from ~1.6 m to infinity. All three cameras can acquire color images through a Bayer color filter array, and the Mastcams can also acquire images through seven science filters. Images are ≤1600 pixels wide by 1200 pixels tall. The Mastcams, mounted on the ~2 m tall Remote Sensing Mast, have a 360° azimuth and ~180° elevation field of regard. Mars Descent Imager is fixed-mounted to the bottom left front side of the rover at ~66 cm above the surface. Its fixed focus lens is in focus from ~2 m to infinity, but out of focus at 66 cm. The f/3 lens has a FOV of ~70° by 52° across and along the direction of motion, with an IFOV of 0.76 mrad. All cameras can acquire video at 4 frames/second for full frames or 720p HD at 6 fps. Images can be processed using lossy Joint Photographic Experts Group and predictive lossless compression.
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Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2017 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2017 Tipo de documento: Article