Rai Choudhuri, Arnab (2011) The origin of the solar magnetic cycle Pramana - Journal of Physics, 77 (1). pp. 77-96. ISSN 0304-4289
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Official URL: http://www.ias.ac.in/pramana/v77/p77/fulltext.pdf
Related URL: http://dx.doi.org/10.1007/s12043-011-0113-4
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: | Article |
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| Source: | Copyright of this article belongs to Indian Academy of Sciences. |
| Keywords: | Sun: Activity; Sun: Magnetic Fields; Sunspots |
| ID Code: | 66540 |
| Deposited On: | 24 Oct 2011 08:26 |
| Last Modified: | 18 May 2016 14:02 |
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