A case study using simulations IRM and CCE observations demonstrates that transient magnetospheric events correspond to pressure pulses in the magnetosheath, inward bow shock motion, and magnetopause compression. Statistical surveys indicate that the magnetosheath magnetic field orientation rarely remains constant during periods of magnetopause and bow shock motion (both characterized by periods of 1 to 10 min). There is no tendency for bow shock motion to occur for southward interplanetary magnetic field (IMF) orientations.


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    Titel :

    Magnetosheath magnetic field variability


    Beteiligte:
    Sibeck, D. G. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1994-07-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Magnetosheath Magnetic Field Variability

    Sibeck, D.G. | Online Contents | 1994


    Magnetosheath Magnetic Field Variability

    Sibeck, D. G. / COSPAR; Interdisciplinary Scientific Commission D | British Library Conference Proceedings | 1994


    Search for Plasma and Magnetic Field Cavities in Magnetosheath

    Turk, F. / Kaymaz, Z. / Sibeck, D. G. et al. | British Library Conference Proceedings | 2003


    Search for plasma and magnetic field cavities in magnetosheath

    Türk, Filiz / Kaymaz, Zerefşan / Sibeck, David G | Elsevier | 2002