Distributed versus tachocline dynamos
Astrophysics
2007-05-23 v1
Abstract
Arguments are presented in favor of the idea that the solar dynamo may operate not just at the bottom of the convection zone, i.e. in the tachocline, but it may operate in a more distributed fashion in the entire convection zone. The near-surface shear layer is likely to play an important role in this scenario.
Cite
@article{arxiv.astro-ph/0512638,
title = {Distributed versus tachocline dynamos},
author = {Axel Brandenburg},
journal= {arXiv preprint arXiv:astro-ph/0512638},
year = {2007}
}
Comments
4 pages, 2 figures, in Solar activity: exploration, understanding and prediction, ed: H. Lundstedt, ESA, ESTEC Noordwijk