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File:Water equivalent hydrogen abundance in the high latitudes of Mars.jpg: Revision history

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31 October 2018

  • curprev 15:5715:57, 31 October 2018 Suitupandshowup talk contribs 820 bytes +820 This map displays the proportion of water ice present in the upper meter of the Martian surface within 30 degrees of the poles. The percentages are derived through stochiometric calculations based on epithermal neutron fluxes. These fluxes were detecte...
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