Turbulent diamagnetism and generation of the mean large-scale magnetic field of the Galaxy

Details Turbulent diamagnetism and generation of the mean large-scale magnetic field of the Galaxy Turbulent diamagnetism and generation of the mean large-scale magnetic field of the Galaxy

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992maggi...3...23z&link_type=abstract

Magnitnaia Gidrodinamika (ISSN 0025-0015), no. 3, p. 23-28.

Physics

Diamagnetism, Dynamo Theory, Galactic Rotation, Interstellar Magnetic Fields, Magnetohydrodynamic Turbulence, Angular Velocity, Magnetic Diffusion, Plasma Turbulence, Plasma-Electromagnetic Interaction

Scientific paper

The large-scale magnetic field in the galactic disk is generated by a
dynamo process determined by differential rotation and helicity. The
turbulent diamagnetism resulting from the spacial inhomogeneity of the
turbulence of galactic matter is shown to inhibit large-scale field
generation and to change its behavior near the Galaxy surface.

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