Computer Science
Scientific paper
Jun 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980p%26ss...28..609a&link_type=abstract
Planetary and Space Science, vol. 28, June 1980, p. 609-615.
Computer Science
7
Interplanetary Magnetic Fields, Magnetic Dipoles, Magnetic Field Configurations, Dynamo Theory, Lines Of Force, Ring Currents, Three Dimensional Models
Scientific paper
A three-dimensional model of the magnetic field configuration in the heliosphere is constructed by assuming that the interplanetary magnetic field consists of four components, (1) the solar dipole, (2) a large number of small spherical dipoles located along an equatorial circle just inside the sun (representing the magnetic field line arcade), (3) the field of the poloidal current system generated by the solar unipolar induction, and (4) the field of an extensive current disc around the sun lying in the ecliptic plane. The magnetic field intensity at a distance of 1 AU (about 20 solar radii above the ecliptic plane) is normalized to fit the observed spiral configuration.
Akasofu Syuh-Ichi
Gray Perry C.
Lee Clarence L.
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