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.

The gnevyshev Gap: a review for space weather

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.
2003
IFSI - Istituto di fisica dello spazio interplanetario
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/169030
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