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Mars’ Magnetism and Its Interaction with the Solar Wind pp 33–114Cite as

The Plasma Environment of Mars

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Part of the book series: Space Sciences Series of ISSI ((SSSI,volume 18))

Abstract

When the supersonic solar wind reaches the neighborhood of a planetary obstacle it decelerates. The nature of this interaction can be very different, depending upon whether this obstacle has a large-scale planetary magnetic field and/or a well-developed atmosphere/ionosphere. For a number of years significant uncertainties have existed concerning the nature of the solar wind interaction at Mars, because of the lack of relevant plasma and field observations. However, measurements by the Phobos-2 and Mars Global Surveyor (MGS) spacecraft, with different instrument complements and orbital parameters, led to a significant improvement of our knowledge about the regions and boundaries surrounding Mars.

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Authors and Affiliations

  1. Atm Oc & Space Sciences, University of Michigan, 1416 Space Research, Ann Arbor, MI, 48109, USA

    A. F. Nagy

  2. Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA

    D. Winterhalter

  3. Max-Planck-Institut für Aeronomie, Max-Planck-Str. 2, 37191, Katlenburg-Lindau, Germany

    K. Sauer, E. Dubinin & W. I. Axford

  4. University of Kansas, Lawrence, USA

    T. E. Cravens

  5. Bay Area Res Corp, Orinda, CA, 94563, USA

    S. Brecht

  6. Centre d’Etude Spatiale des Rayonnements/CNRS, Toulouse, France

    C. Mazelle & C. Bertucci

  7. Department of Physics, Catholic University of America, Washington, D.C., 20064, USA

    D. Crider

  8. Geophysical Research, Finnish Meteorological Institute, Helsinki, Finland

    E. Kallio

  9. Space Research Institute, Russian Academy of Sciences, Ul. Profsoyuznaya 84/32, Moscow, Russia, GSP-7 117997

    A. Zakharov, M. Verigin & G. Kotova

  10. de l’Environnement, LPCE/CNRS, Laboratoire de Physique et Chimie, 3A, Ave. de la Recherche Scientifique, F-45071, Orleans Cedex 2, France

    J. G. Trotignon

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Editors and Affiliations

  1. Jet Propulsion Laboratory, California Institute of Technology, USA

    Daniel Winterhalter

  2. NASA/Goddard Space Flight Center, USA

    Mario Acuña

  3. Space Research Institute, Moscow, Russia

    Alexander Zakharov

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Nagy, A.F. et al. (2004). The Plasma Environment of Mars. In: Winterhalter, D., Acuña, M., Zakharov, A. (eds) Mars’ Magnetism and Its Interaction with the Solar Wind. Space Sciences Series of ISSI, vol 18. Springer, Dordrecht. https://doi.org/10.1007/978-0-306-48604-3_2

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