Data di Pubblicazione:
2003
Abstract:
The 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 wich a decrease in solar atmospheric activity is observed) in the time history of Space Weather parameters.
Tipologia CRIS:
01.01 Articolo in rivista
Elenco autori:
Storini, Marisa
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