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Solar and planetary dynamos: comparison and recent developments

Published online by Cambridge University Press:  01 September 2008

K. Petrovay
K. Petrovay*
Affiliation:
Eötvös University, Department of Astronomy H-1518 Budapest, Pf. 32., Hungary email: K.Petrovay@astro.elte.hu
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Abstract

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While obviously having a common root, solar and planetary dynamo theory have taken increasingly divergent routes in the last two or three decades, and there are probably few experts now who can claim to be equally versed in both. Characteristically, even in the fine and comprehensive book “The magnetic Universe” (Rudiger & Hollerbach 2004), the chapters on planets and on the Sun were written by different authors. Separate reviews written on the two topics include Petrovay (2000), Charbonneau (2005), Choudhuri (2008) on the solar dynamo and Glatzmaier (2002), Stevenson (2003) on the planetary dynamo. In the following I will try to make a systematic comparison between solar and planetary dynamos, presenting analogies and differences, and highlighting some interesting recent results.

Keywords

magnetic fieldsMHDplasmasturbulenceSun: magnetic fieldsSun: interiorEarthplanets and satellites: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S257: Universal Heliophysical Processes , September 2008 , pp. 71 - 81
Copyright
Copyright © International Astronomical Union 2009

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