Double ring algorithm of solar active region eruptions within the framework of kinematic dynamo model
Solar and Stellar Astrophysics
2014-04-08 v1
Abstract
Recent results indicate that the Babcock-Leighton mechanism for poloidal field creation plays an important role in the solar cycle. However, modelling this mechanism has not always correctly captured the underlying physics. In particular, it has been demonstrated that using a spatially distributed near-surface alpha-effect to parametrize the Babcock-Leighton mechanism generates results which do not agree with observations. Motivated by this, we are developing a physically more consistent model of the solar cycle in which we model poloidal field creation by the emergence and flux dispersal of double-rings structures. Here we present preliminary results from this new dynamo model.
Cite
@article{arxiv.1302.3133,
title = {Double ring algorithm of solar active region eruptions within the framework of kinematic dynamo model},
author = {Soumitra Hazra and Dibyendu Nandy},
journal= {arXiv preprint arXiv:1302.3133},
year = {2014}
}
Comments
To appear in proceedings of the ISSTP 2012, 4 Pages,3 figures