Studies of the Martian bow shock response to the variation of the magnetosphere dimensions according to Taus and Magma measurements aboard the Phobos 2 orbiter

M. I. Verigin, G. A. Kotova, A. P. Remizov, N. M. Shutte, K. Schwingenschuh, W. Riedler, T. L. Zhang, H. Rosenbauer, K. Szegö, M. Tatrallyay, V. Styazhkin

Research output: Contribution to journalArticle

9 Citations (Scopus)

Abstract

A self-consistent quantitative model is presented which describes the planetary bow shock motion and its shape variation due to variations of the external plasma flow parameters and the magnetopause shape. This model is applied to the analysis of the Martian bow shock motions and for the explanation of its unusual properties.

Original languageEnglish
Pages (from-to)155-158
Number of pages4
JournalAdvances in Space Research
Volume20
Issue number2
DOIs
Publication statusPublished - Jan 1 1997

ASJC Scopus subject areas

  • Aerospace Engineering
  • Astronomy and Astrophysics
  • Geophysics
  • Atmospheric Science
  • Space and Planetary Science
  • Earth and Planetary Sciences(all)

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    Verigin, M. I., Kotova, G. A., Remizov, A. P., Shutte, N. M., Schwingenschuh, K., Riedler, W., Zhang, T. L., Rosenbauer, H., Szegö, K., Tatrallyay, M., & Styazhkin, V. (1997). Studies of the Martian bow shock response to the variation of the magnetosphere dimensions according to Taus and Magma measurements aboard the Phobos 2 orbiter. Advances in Space Research, 20(2), 155-158. https://doi.org/10.1016/S0273-1177(97)00526-7