Choudhuri, Arnab Rai (2011) The origin of the solar magnetic cycle. In: Pramana - Journal of Physics, 77 (1, SI). pp. 77-96.
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Official URL: http://www.springerlink.com/content/b568u758737460...
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.
Item Type: | Journal Article |
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Publication: | Pramana - Journal of Physics |
Publisher: | Indian Academy of Sciences |
Additional Information: | Copyright of this article belongs to Indian Academy of Sciences. |
Keywords: | Sun;activity;Sun;magnetic fields;sunspots |
Department/Centre: | Division of Physical & Mathematical Sciences > Physics |
Date Deposited: | 30 Aug 2011 06:37 |
Last Modified: | 30 Aug 2011 06:37 |
URI: | http://eprints.iisc.ac.in/id/eprint/39951 |
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