Computer Science
Scientific paper
Jul 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kosis..27..604d&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 27, July-Aug. 1989, p. 604-616. In Russian.
Computer Science
Dynamo Theory, Magnetic Dipoles, Neptune (Planet), Planetary Magnetic Fields, Uranus (Planet), Magnetohydrodynamics, Neptune Satellites, Planetary Cores, Uranus Satellites
Scientific paper
The expected intensity of the dipole magnetic field of Neptune is determined in the framework of the 'numerical law' of the precession-dynamo model. Attention is also given to possible causes of the extraordinarily large values of the inclination and eccentricity of the dipole of Uranus in comparison with the dipoles of Jupiter and the earth.
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