Intrinsic magnetic field of a solar convective element

Details Intrinsic magnetic field of a solar convective element Intrinsic magnetic field of a solar convective element

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980avest..13..187k&link_type=abstract

(Astronomicheskii Vestnik, vol. 13, July-Sept. 1979, p. 187, 188.) Solar System Research, vol. 13, no. 3, Jan. 1980, p. 145, 146

Physics

Convective Flow, Magnetohydrodynamic Flow, Solar Magnetic Field, Solar Wind, Dynamo Theory, Hydrodynamic Equations, Solar Physics

Scientific paper

One of the possible mechanisms for generating the initial triggering magnetic fields that are amplified by the solar dynamo mechanism is examined. It is shown that the field which arises during the hydrodynamic motion of the plasma in a convective element has an intensity of from 10 to the -12th power to 10 to the -11th power Oe and forms the regular structure in the sun's outer layers.

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