AbstractThe ability to forecast long-term Space Weather effects needs a good knowledge of solar activity behaviour along the 11-year sunspot cycle. In this paper we concentrate our attention on the so-called maximum activity phase and we discuss the role of the Gnevyshev gap (a time interval in which a decrease in solar atmospheric activity is observed) in the time history of Space Weather parameters.
The GNEVYSHEV gap: A review for space weather
Advances in Space Research ; 31 , 4 ; 895-900
2002-01-01
6 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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