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Towards understanding the global magnetism of the Sun and solar-like stars
Published online by Cambridge University Press: 26 February 2010
Abstract
The Sun and solar-like stars possess intense and cyclic magnetic activity. In order to understand how this comes about we have developed series of 2-D and 3-D models in order to simulate their global dynamics and magnetism. We here report on our latest findings.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Symposium S264: Solar and Stellar Variability: Impact on Earth and Planets , August 2009 , pp. 161 - 170
- Copyright
- Copyright © International Astronomical Union 2010