Article contents
Coronal ejections from convective spherical shell dynamos
Published online by Cambridge University Press: 05 July 2012
Abstract
We present a three-dimensional model of rotating convection combined with a simplified model of a corona in spherical coordinates. The motions in the convection zone generate a large-scale magnetic field which is sporadically ejected into the outer layers above. Our model corona is approximately isothermal, but it includes density stratification due to gravity.
- Type
- Contributed Papers
- Information
- Copyright
- Copyright © International Astronomical Union 2012
References
- 1
- Cited by