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Explaining Jupiter's magnetic field and equatorial jet dynamics

Published:2014-08-11 Issue:15 Volume:41 Page:5410-5419
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Gastine T.¹,Wicht J.¹,Duarte L. D. V.¹²,Heimpel M.³,Becker A.⁴

Affiliation:

1. Max-Planck-Institut für Sonnensystemforschung; Göttingen Germany

2. Laboratoire de Géologie de Lyon, CNRS; Université de Lyon; Lyon France

3. Department of Physics; University of Alberta; Edmonton Alberta Canada

4. Institut für Physik; Universität Rostock; Rostock Germany

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2014GL060814/fullpdf

Reference36 articles.

1. Persistent magnetic wreaths in a rapidly rotating Sun;Brown;Astrophys. J.,2010

2. Ab initio simulations of MgO under extreme conditions;Cebulla;Phys. Rev. B,2014

3. Dynamo scaling laws and applications to the planets;Christensen;Space Sci. Rev.,2010

4. Scaling properties of convection-driven dynamos in rotating spherical shells and application to planetary magnetic fields;Christensen;Geophys. J. Int.,2006

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