Generation of magnetic fields by convection in a rotating sphere, I-Reference-Cited by-同舟云学术

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Generation of magnetic fields by convection in a rotating sphere, I

Published:1981-03 Issue:4 Volume:24 Page:272-283
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:

Cuong P.G.,Busse F.H.

Publisher

Elsevier BV

Subject

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

Reference15 articles.

1. Structure of the F layer and reasons for convection in the Earth's core;Braginsky;Dokl. Akad. Nauk SSSR,1963

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

3. A model of the geodynamo;Busse;Geophys. J.R. Astron. Soc.,1975

4. Generation of planetary magnetism by convection;Busse;Phys. Earth Planet. Inter.,1976

5. Convection in rapidly rotating spherical fluid shells;Busse;Geophys. Astrophys. Fluid Dyn.,1977

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3. Dynamics of the Earth's Core and the Geodynamo;Geophysical Monograph Series;2013-03-29

4. Stellar Convection and Magnetism across the H-R diagram: Theory and Models;EAS Publications Series;2009

5. Geodynamo Simulations—How Realistic Are They?;Annual Review of Earth and Planetary Sciences;2002-05

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