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Solar wind deceleration at Mars and Earth: A comparison

  • T. L. Zhang*
  • , K. Schwingenschuh
  • , W. Riedler
  • , G. Kotova
  • , M. Verigin
  • , M. Tatrallyay
  • , C. T. Russell
  • *Corresponding author for this work
  • Austrian Academy of Sciences
  • Space Research Institute of the Russian Academy of Sciences
  • Wigner Research Centre for Physics

Research output: Contribution to journalArticlepeer-review

Abstract

Phobos 2 plasma measurements have revealed the solar wind deceleration upstream of the Martian terminator bow shock. Earlier studies have shown that the solar wind is decelerated and deflected in the Earth's foreshock region. At Mars, the solar wind decelerated more at duskside than at dawnside. At Earth the solar wind decelerates most upstream of the quasi-parallel bow shock in the foreshock region. In this paper, we investigate and compare the solar wind deceleration at Mars and Earth.

Original languageEnglish
Pages (from-to)133-136
Number of pages4
JournalAdvances in Space Research
Volume20
Issue number2
DOIs
StatePublished - 1997
Externally publishedYes

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