The remarkable success with which gas dynamic models characterize the plasma properties in the magnetosheath has to some degree diverted attention from certain inherently magnetohydrodynamic effects that are expected to introduce important modifications. Three recent aspects of magnetosheath observations: a slow mode structure near the subsolar point, flows at speeds in excess of the solar wind speed, and the shape of the internal boundary, i.e., the magnetopause, provide examples of inherently magnetohydrodynamic (MHD) effects.


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    Titel :

    Consequences of magnetohydrodynamic processes for large scale flow in the magnetosheath


    Beteiligte:
    Kivelson, M. G. (Autor:in) / Chen, S.-H. (Autor:in) / Southwood, D. J. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.07.1994



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :



    Consequences of Magnetohydrodynamic Processes for Large Scale Flow in the Magnetosheath

    Kivelson, M. G. / Chen, S.-H. / Southwood, D. J. et al. | British Library Conference Proceedings | 1994


    Consequences of magnetohydrodynamic processes for large scale flow in the magnetosheath

    Kivelson, M.G. / Chen, S.-H. / Southwood, D.J. | Elsevier | 1994



    Gasdynamic and Magnetohydrodynamic Modeling of the Magnetosheath: A Tutorial

    Spreiter, J. R. / Stahara, S. S. / COSPAR; Interdisciplinary Scientific Commission D | British Library Conference Proceedings | 1994