On the influence of density waves on galactic magnetic fields

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Density Distribution, Dynamo Theory, Interstellar Magnetic Fields, Spiral Galaxies, Astronomical Models, Field Strength, Galactic Evolution, Shock Waves

Scientific paper

The growth rate for the bisymmetric magnetic field in the two-dimensional swing-excitation model (Chiba and Tosa, 1990) is derived. A possible explanation of the observed correlation between the magnetic field strength and the strength of the density wave shock is proposed. Three different mechanisms of magnetic field amplification by a density wave are elucitated.

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