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      Solar panel clearing events, dust devil tracks, and in-situ vortex detections on Mars

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      Icarus
      Elsevier BV

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          Abstract

          <p class="first" id="P1">Spirit rover solar array data, which if publicly-archived would provide a useful window on Mars meteorology, shows dust-clearing events coinciding with the onset of dust devil season in three Mars years. The recurrence interval of 100–700 days is consistent with the extrapolation of Pathfinder and Phoenix vortex encounters indicated by pressure drops of ~6–40 Pa (similar to laboratory measurements of dust lifting threshold) and with observed areas and rates of generation of dust devil tracks on Mars. </p>

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          Most cited references23

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          Overview of the Mars Pathfinder Mission: Launch through landing, surface operations, data sets, and science results

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            Active dust devils in Gusev crater, Mars: Observations from the Mars Exploration Rover Spirit

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              • Record: found
              • Abstract: not found
              • Article: not found

              Convective vortices and dust devils at the Phoenix Mars mission landing site

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                Author and article information

                Journal
                Icarus
                Icarus
                Elsevier BV
                00191035
                March 2015
                March 2015
                : 248
                :
                : 162-164
                Article
                10.1016/j.icarus.2014.10.034
                6350794
                30705464
                adeea25f-112e-4067-a22f-31606f361ea6
                © 2015
                History

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