Three-dimensional kinematic dynamos with equatorial symmetry: Application to the magnetic fields of Uranus and Neptune-Reference-Cited by-同舟云学术

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Three-dimensional kinematic dynamos with equatorial symmetry: Application to the magnetic fields of Uranus and Neptune

Published:1997-06 Issue:1-2 Volume:102 Page:105-122
ISSN:0031-9201
Container-title:Physics of the Earth and Planetary Interiors
language:en
Short-container-title:Physics of the Earth and Planetary Interiors

Author:

Holme Richard

Publisher

Elsevier BV

Subject

Space and Planetary Science,Physics and Astronomy (miscellaneous),Geophysics,Astronomy and Astrophysics

Reference51 articles.

1. A class of self-sustaining dissipative spherical dynamos;Backus;Ann. Phys.,1958

2. Homogeneous dynamos and terrestrial magnetism;Bullard;Philos. Trans. R. Soc. London A,1954

3. Generation of magnetic fields by fluid motions of global scale;Bullard;Geophys. Astrophys. Fluid Dyn.,1977

4. A model of the geodynamo;Busse;Geophys. J. Roy. Astron. Soc.,1975

5. Generation of planetary magnetism by convection;Busse;Phys. Earth Planet. Int.,1976

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1. Planetary Magnetic Fields;Magnetospheres in the Solar System;2021-04-23

2. The optimal kinematic dynamo driven by steady flows in a sphere;Journal of Fluid Mechanics;2018-01-25

3. Ultracondensed Matter by Dynamic Compression;2017

4. Theory of the Geodynamo;Treatise on Geophysics;2015

5. Planetary Dynamos and Helicities;Magnetic Helicity in Space and Laboratory Plasmas;2013-03-19

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