A nonlinear dynamo for galaxies and accretion disks.

Details A nonlinear dynamo for galaxies and accretion disks. A nonlinear dynamo for galaxies and accretion disks.

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nawg.1996..282b&link_type=abstract

Nachr. Akad. Wiss. Göttingen II, Jahrg. 1996, Nr. 4, p. 282 - 288

Physics

Spiral Galaxies: Dynamo Theory, Accretion Disks: Dynamo Theory

Scientific paper

The large scale magnetic fields of spiral galaxies and accretion disks are ascribed to a dynamo. Nonlinear dynamo calculations including magnetic buoyancy and α-quenching show that the most preferred magnetic field is of quadrupolar type. This agrees with the observations. In several cases dipolar or oscillating fields occur, where the latter oscillate in magnetic energy and the symmetry property.

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