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• W2109612288 abstract "After summarizing the relevant observational data, we discuss how a study of flux tube dynamics in the solar convection zone helps us to understand the formation of sunspots. Then we introduce the flux transport dynamo model and assess its success in modelling both the solar cycle and its departures from strictly periodic behaviour." @default.
• W2109612288 created "2016-06-24" @default.
• W2109612288 creator A5052640104 @default.
• W2109612288 date "2011-07-01" @default.
• W2109612288 modified "2023-09-23" @default.
• W2109612288 title "The origin of the solar magnetic cycle" @default.
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• W2109612288 doi "https://doi.org/10.1007/s12043-011-0113-4" @default.
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