No CrossRef data available.
Article contents
Alpha-Quenched Alpha-Lambda Dynamos and the Excitation of Nonaxisymmetric Magnetic Fields
Published online by Cambridge University Press: 19 July 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
We present calculations showing how stable nonaxisymmetric magnetic fields may be excited in an alpha-quenched mean field dynamo in a deep spherical shell. The large scale velocity fields (differential rotation, meridional circulation) are determined by solving the axisymmetric Navier-Stokes equation, neglecting the Lorentz force but including a term parameterizing the turbulent Reynolds stresses.
- Type
- 4. Late-Type and Other Stars
- Information
- Copyright
- Copyright © Kluwer 1993
References
Barker, D.M.: 1993,
Proceedings of N.A.T.O. A.S.I.: Theory of Solar and Planetary Dynamos
, submitted
Google Scholar
Moss, D.: 1992, in Tuominen, I., Moss, D. & Rüdiger, G., ed(s).,
The Sun and cool stars: activity, magnetism, dynamos
, Springer-Verlag: Berlin, 112
Google Scholar
Rädler, K.-H., Wiedemann, E., Brandenburg, A., Meinel, R., & Tuominen, I.: 1990,
A&A
239, 413
Google Scholar
Rüdiger, G.: 1989,
Differential Rotation and Stellar Convection
, Gordon and Breach: New York
CrossRefGoogle Scholar
You have
Access