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Sylvain Piqueux and Philip R. Christensen Visible and thermal infrared observations of the Martian surface during three Phobos shadow transits Geophysical Research Letters 39

Version of Record online: 14 NOV 2012 | DOI: 10.1029/2012GL053352

Key Points

  • THEMIS VIS and IR observations of 3 Phobos transits show no surface cooling
  • Thermal modeling requires that the top material is coarser than dust
  • No surface dust is consistent with other remote sensing techniques

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