Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..289s&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Mar.-Apr. 1985, p. 289-296. In Russian.
Astronomy and Astrophysics
Astronomy
1
Astronomical Models, Dynamo Theory, Earth Core, Magnetic Dipoles, Spheres, Strata, Kinematics, Magnetic Field Configurations, Poloidal Flux, Toroids
Scientific paper
A kinematic dynamo model is proposed which reflects the main structural features of the earth's core and allows a determination of poloidal velocity modes which provide for the most efficient magnetic-field generation. Magnetic-field generation in a partially stratified core with velocities of toroidal motion of the order of the western-drift velocity of magnetic anomalies of the earth is demonstrated. The poloidal-flow velocity sufficient in this model to generate the earth's dipole magnetic field is 300-1000 times less than the western-drift velocity. It is concluded that the proposed model makes it possible to determine optimal orientations for arbitrary poloidal velocity modes.
Kropachev Eh. P.
Serebrianaia P. M.
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