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SHARAD detection and characterization of subsurface water ice deposits in Utopia Planitia, Mars

  • Published:2016-09-28 Issue:18 Volume:43 Page:9484-9491
  • ISSN:0094-8276
  • Container-title:Geophysical Research Letters
  • language:en
  • Short-container-title:Geophys. Res. Lett.

Author:

Stuurman C. M.12,Osinski G. R.23,Holt J. W.1,Levy J. S.1,Brothers T. C.14ORCID,Kerrigan M.2,Campbell B. A.15

Affiliation:

1. Institute for Geophysics; University of Texas at Austin; Austin Texas USA

2. Centre for Planetary Science and Exploration, Department of Earth Sciences; University of Western Ontario; London Ontario Canada

3. Department of Physics and Astronomy; University of Western Ontario; London Ontario Canada

4. Malin Space Science Systems; San Diego California USA

5. Smithsonian Institution; Washington District of Columbia USA

Funder

Natural Sciences and Engineering Research Council of Canada

NSERC/CSA/MDA Industrial Research Chair in Planetary Geology

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference39 articles.

1. Widespread excess ice in Arcadia Planitia, Mars;Bramson;Geophys. Res. Lett.,2015

2. Distribution of mid-latitude ground ice on Mars from new impact craters;Byrne;Science,2009

3. Surface clutter and echo location analysis for the interpretation of SHARAD data from Mars;Choudhary;Geosci. Remote Sens. Lett.,2016

4. JMARS-A planetary GIS;Christensen;Eos Trans. AGU,2009
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