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Paper detail

The origin of the solar magnetic cycle

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.

preprint2011arXivOpen access
Arnab Rai Choudhuri
astro-ph.SR
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Arnab Rai Choudhuri

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