Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8139102 | Journal of Atmospheric and Solar-Terrestrial Physics | 2018 | 5 Pages |
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.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Arnab Rai Choudhuri,