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Study on the O+ ion distribution and escape in Martian atmosphere

  • Jiankui Shi*
  • , Zhenxing Liu
  • , Klaus Torkar
  • , Tielong Zhang
  • , Malcolm Dunlop
  • *Corresponding author for this work
  • Chinese Academy of Sciences
  • Austrian Academy of Sciences
  • Rutherford Appleton Laboratory

Research output: Chapter in Book/Report/Conference proceedingChapterpeer-review

Abstract

In this paper, we have considered the view that the Martian magnetic moment has been gradually decreasing from the past to the present, and have calculated the O+ ion flux distribution along magnetic field lines and the escaping ion flux in the Martian tail with different assumed Martian magnetic moments. The results show that the O+ ions flux along magnetic field lines decreases with increasing distance to Mars; that the ion flux along the field line decreases more rapidly if the magnetic moment is larger; and that the larger the magnetic moment, the smaller the ion flux in the Martian tail becomes. The escaping ion flux depends on the Z-coordinate in the Martian tail. With decreasing magnetic moment, the escaping ion flux in the Martian tail is increasing. The results are significant for studying the ion loss from Mars.

Original languageEnglish
Title of host publicationAdvances in Geosciences
Subtitle of host publicationVolume 19: Planetary Science (PS)
PublisherWorld Scientific Publishing Co.
Pages251-260
Number of pages10
ISBN (Electronic)9789812838162
ISBN (Print)9812838155, 9789812838155
DOIs
StatePublished - 1 Jan 2010
Externally publishedYes

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