The symmetry properties of planetary magnetic fields

Author:

Rädler Karl-Heinz,Ness Norman F.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference35 articles.

1. The main magnetic field of Jupiter;Acuña;J. Geophys. Res.,1976

2. On Cowling's theorem of the impossibility of self-sustained axisymmetric homogeneous dynamos;Backus;Proc. Natl. Acad. Sci. U. S. A.,1956

3. Thermal core-mantle interactions;Bloxham;Nature,1987

4. Self excitation of a magnetic field during the motion of a highly conducting fluid;Braginski;Sov. Phys. JETP,1964

5. On the conditions favoring axisymmetric or non-axisymmetric magnetic field modes in mean-field dynamo models;Brandenburg;Geophys. Astrophys. Fluid Dyn.,1989

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2. Planetary Magnetism;Treatise on Geophysics;2015

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4. Planetary Magnetism;Treatise on Geophysics;2007

5. Astrophysical magnetic fields and nonlinear dynamo theory;Physics Reports;2005-10

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