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Autor:
Usoskin, I. G. (I. G.), Solanki, S. K. (S. K.), Krivova, N. A. (N. A.), Hofer, B. (B.), Kovaltsov, G. A. (G. A.), Wacker, L. (L.), Brehm, N. (N.), Kromer, B. (B.)
Aims: The 11-year solar cycle (Schwabe cycle) is the dominant pattern of solar magnetic activity reflecting the oscillatory dynamo mechanism in the Sun’s convection zone. Solar cycles have been directly observed since 1700, while indirect proxy dat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2423::db495ac27d8b7840ff1ec03866ca9987
http://urn.fi/urn:nbn:fi-fe2021060233123
http://urn.fi/urn:nbn:fi-fe2021060233123
