The dynamo theory of plasma turbulence wave in rotating celestial bodies

Details The dynamo theory of plasma turbulence wave in rotating celestial bodies The dynamo theory of plasma turbulence wave in rotating celestial bodies

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.113..303t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 113, no. 2, July 1985, p. 303-316.

Astronomy and Astrophysics

Astrophysics

3

Celestial Bodies, Dynamo Theory, Magnetohydrodynamic Turbulence, Magnetohydrodynamic Waves, Rotating Bodies, Angular Velocity, Planetary Magnetic Fields, Solar Rotation, Stellar Magnetic Fields, Stellar Rotation

Scientific paper

The various modes of plasma turbulence waves (including MHD waves) are easily excited under cosmic circumstances. In this paper, if the celestial bodies are considered to rotate, there is a source term generated for the magnetic-induced equation by the excited plasma turbulence waves. If the turbulent field is expanded in the Fourier series and rotation velocity is included, the dynamo equation for turbulent waves is obtained. Also obtained are the solutions of various wave forms corresponding to different rotation velocities. The magnetic fields in the sun, planets, and other celestial bodies are discussed.

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