Choudhuri, Arnab Rai (2018) Flux transport dynamo: From modelling irregularities to making predictions. In: JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 176 (SI). pp. 5-9.
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Abstract
The flux transport dynamo, in which the poloidal magnetic field is generated by the Babcock Leighton mechanism and the meridional circulation plays a crucial role, has emerged as an attractive model for the solar cycle. Based on theoretical calculations done with this model, we argue that the fluctuations in the Babcock Leighton mechanism and the fluctuations in the meridional circulation are the most likely causes of the irregularities of the solar cycle. With our increased theoretical understanding of how these irregularities arise, it can be possible to predict a future solar cycle by feeding the appropriate observational data in a theoretical dynamo model.
Item Type: | Journal Article |
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Publication: | JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS |
Publisher: | PERGAMON-ELSEVIER SCIENCE LTD |
Additional Information: | Copy right for this article belong to PERGAMON-ELSEVIER SCIENCE LTD, THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND |
Keywords: | Dynamo; Solar cycle |
Department/Centre: | Division of Physical & Mathematical Sciences > Physics |
Date Deposited: | 27 Sep 2018 14:48 |
Last Modified: | 27 Sep 2018 14:48 |
URI: | http://eprints.iisc.ac.in/id/eprint/60747 |
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