AbstractThe ionospheres of Venus and Mars have been explored by a number of spacecraft. It is now widely recognized that. Venus and Mars possess no significant intrinsic magnetic fields, and that the solar wind interacts directly with the upper atmospheres of the planets. The structure and dynamics of the ionospheres are strongly controlled by the solar wind. In situ measurements of Venus and Mars revealed that the ionospheres are often filled with solar wind-induced magnetic field. In addition, the Martian ionosphere is also influenced by the crustal magnetic field at least in some regions, which makes the ionospheric processes at Mars even more complicated than those at Venus. Current understanding of the ionospheric processes of Venus and Mars is presented based on the observational and theoretical studies of the structure, dynamics, and the ionospheric magnetic field of the ionospheres of Venus and Mars.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    The ionospheres of Venus and Mars


    Beteiligte:
    Shinagawa, H. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 33 , 11 ; 1924-1931


    Erscheinungsdatum :

    2003-06-08


    Format / Umfang :

    8 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




    The ionospheres of Venus and Mars

    Shinagawa, H. | Online Contents | 2004


    The Ionospheres of Venus and Mars

    Shinagawa, H. / International Council of Scientific Unions | British Library Conference Proceedings | 2004


    Ionospheres of Venus and Mars: a Comparative Study

    Mahajan, K. K. / Dwivedi, A. K. / International Council of Scientific Unions | British Library Conference Proceedings | 2004


    Ionospheres of Venus and Mars: a comparative study

    Mahajan, K.K. | Online Contents | 2004


    Ionospheres of Venus and Mars: a comparative study

    Mahajan, K.K. / Dwivedi, A.K. | Elsevier | 2003