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Low-dimensional models of stellar and galactic dynamos

Published online by Cambridge University Press:  01 November 2008

Dimitry Sokoloff  and
S. Nefyodov
Dimitry Sokoloff
Affiliation:
Department of Physics, Moscow State University, Moscow, 119991, Russia email: sokoloff@dds.srcc.msu.su; rainbow84@rambler.ru
S. Nefyodov
Affiliation:
Department of Physics, Moscow State University, Moscow, 119991, Russia email: sokoloff@dds.srcc.msu.su; rainbow84@rambler.ru
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Abstract

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A regular method how to simplify dynamo model for a particular celestial body up to a dynamical system is suggested. Dynamical system obtained occurs specific for a thin galactic disc, a fully convective star and a thin convective shell.

Keywords

Magnetic fields – convection – stars: low-mass
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S259: Cosmic Magnetic Fields: From Planets, to Stars and Galaxies , November 2008 , pp. 419 - 420
Copyright
Copyright © International Astronomical Union 2009

References

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