AbstractStarting with our elliptical cross-section model for the study of the magnetic topology of magnetic clouds (MCs) in the interplanetary medium, we develop an analytical approach to the behavior of the Dst index at the recovery phase of a geomagnetic storm.Assuming an axially symmetric ring current, we estimate its physical parameters during that recovery phase of the storm-time. We compare the theoretical and measured Dst indexes in two intense geomagnetic storms (Dst <–100 nT), both associated with MCs.


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    Titel :

    The relationship between the recovery phase of geomagnetic storms and the magnetic clouds


    Beteiligte:
    Hidalgo, M.A. (Autor:in) / Cantalapiedra, I.R. (Autor:in) / Sequeiros, J. (Autor:in) / Cid, C. (Autor:in) / Nieves-Chinchilla, T. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 35 , 3 ; 426-428


    Erscheinungsdatum :

    2005-03-29


    Format / Umfang :

    3 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch





    The relationship between the recovery phase of geomagnetic storms and the magnetic clouds

    Hidalgo, M. A. / Cantalapiedra, I. R. / Sequeiros, J. et al. | British Library Conference Proceedings | 2005


    Stream-Interacting Magnetic Clouds Causing Very Intense Geomagnetic Storms

    Lago, A. D. / Gonzalez, W. D. / de Gonzalez, A. L. C. et al. | British Library Conference Proceedings | 2002