Diurnal variations of energetic particle radiation at the surface of Mars as observed by the Mars Science Laboratory Radiation Assessment Detector

Scot C.R. Rafkin*, Cary Zeitlin, Bent Ehresmann, Don Hassler, Jingnan Guo, Jan Köhler, Robert Wimmer-Schweingruber, Javier Gomez-Elvira, Ari-Matti Harri, Henrik Kahanpää, David E. Brinza, Gerald Weigle, Stephan Böttcher, Eckart Böhm, Söenke Burmeister, Cesar Martin, Guenther Reitz, Francis A. Cucinotta, Myung-Hee Kim, David GrinspoonMark A. Bullock, Arik Posner, MSL Science Team

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

45 Citations (Scopus)

Abstract

The Radiation Assessment Detector onboard the Mars Science Laboratory rover Curiosity is detecting the energetic particle radiation at the surface of Mars. Data collected over the first 350 Martian days of the nominal surface mission show a pronounced diurnal cycle in both the total dose rate and the neutral particle count rate. The diurnal variations detected by the Radiation Assessment Detector were neither anticipated nor previously considered in the literature. These cyclic variations in dose rate and count rate are shown to be the result of changes in atmospheric column mass driven by the atmospheric thermal tide that is characterized through pressure measurements obtained by the Rover Environmental Monitoring Station, also onboard the rover. In addition to bulk changes in the radiation environment, changes in atmospheric shielding forced by the thermal tide are shown to disproportionately affect heavy ions compared to H and He nuclei.
Original languageEnglish
Pages (from-to)1345-1358
Number of pages14
JournalJournal of Geophysical Research - Planets
Volume119
Issue number6
Early online date18 Jun 2014
DOIs
Publication statusPublished - Jun 2014

Bibliographical note

The authors are extremely grateful for the comments from the anonymous reviewers who greatly improved the manuscript. The data used in this paper may be retrieved from the NASA Planetary Data System. RAD is supported by NASA under JPL subcontract 1273039 to Southwest Research Institute and in Germany by Deutsches Zentrum fur Luft‐und Raumfahrt (DLR) and DLR's Space Administration grants 50QM0501 and 50QM1201 to the Christian‐Albrechts University, Kiel. A portion of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

Keywords

  • Mars
  • Radiation
  • space weather
  • atmosphere
  • Mars Science Laboratory

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