Abstract In 2003, geomagnetic activity was found to be considerably higher than in any other year of the current solar cycle. This was caused by the time coincidence of large low-latitude coronal holes and a significant burst of the flare and eruptive activity of the Sun. The features of recent intensification of the activity are discussed, and the long-period behavior of indices of the geomagnetic activity in the 23rd and previous cycles is compared. The large magnetic storms in October–November 2003 are analyzed in more detail.


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    Titel :

    Unusually high geomagnetic activity in 2003


    Beteiligte:
    Belov, A. V. (Autor:in) / Gaidash, S. P. (Autor:in) / Ivanov, K. G. (Autor:in) / Kanonidi, Kh. D. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    2004




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Print


    Sprache :

    Englisch


    Schlagwörter :

    Klassifikation :

    BKL:    55.60 Raumfahrttechnik / 39.00 Astronomie: Allgemeines / 50.93 Weltraumforschung
    Lokalklassifikation TIB:    770/3520/8000



    Unusually high geomagnetic activity in 2003

    Belov, A. V. / Gaidash, S. P. / Ivanov, K. G. et al. | Springer Verlag | 2004


    Geomagnetic Response to Solar Activity

    Mclntosh, Patrick S. / Dryer, Murray | AIAA | 1972


    Geomagnetic activity and solar cycles

    Silbergleit, V.M. / Larocca, P.A. | Elsevier | 2003


    IMF control of geomagnetic activity

    McPherron, R.L. / Baker, D.N. / Bargatze, L.F. et al. | Elsevier | 1989


    IMF control of geomagnetic activity

    Mcpherron, R. L. / Bargatze, L. F. / Holzer, R. E. et al. | NTRS | 1988