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Physik des erdnahen Weltraums pp 409–455Cite as

Geosphärenstürme

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Zusammenfassung

Als Geosphärensturm bezeichnen wir eine Periode stark erhöhter Dissipation von Sonnenwindenergie in der Raumumgebung der Erde. Solche Ereignisse dauern typischerweise 1 bis 3 Tage und sind durch Energiedissipationsraten von bis zu 1012 W gekennzeichnet. Dies entspricht einem Vielfachen des normalen Energietransfers Sonnenwind-Magnetosphäre.

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Literaturhinweise

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Author information

Authors and Affiliations

  1. Institut für Astrophysik und Extraterrestrische Physik, Universität Bonn, Auf dem Hügel 71, 53121, Bonn, Deutschland

    Professor Gerd W. Prölss

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  1. Professor Gerd W. Prölss
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© 2001 Springer-Verlag Berlin Heidelberg

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Prölss, G.W. (2001). Geosphärenstürme. In: Physik des erdnahen Weltraums. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-97903-3_8

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  • DOI: https://doi.org/10.1007/978-3-642-97903-3_8

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-97904-0

  • Online ISBN: 978-3-642-97903-3

  • eBook Packages: Springer Book Archive

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