Correlative properties of self-exciting fluctuative magnetic fields

Details Correlative properties of self-exciting fluctuative magnetic fields Correlative properties of self-exciting fluctuative magnetic fields

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.251..557k&link_type=abstract

In ESA Proceedings of the Joint Varenna-Abastumani International School and Workshop on Plasma Astrophysics p 557-561 (SEE N87-

Astronomy and Astrophysics

Astrophysics

8

Correlation Coefficients, Dynamo Theory, Interstellar Magnetic Fields, Turbulent Flow, Asymptotic Methods, High Reynolds Number, Magnetohydrodynamic Flow

Scientific paper

Correlation function of the magnetic fields excited in a reflectionally symmetrical shortcorrelated turbulent flow is constructed. It is based on an asymptotical solution valid at large magnetic Reynolds numbers Rm. Two magnetic correlation scales appear: l×Rm-1/2 and l×Rm-1/4 in addition to l, where l is a basic scale of the turbulence. The results are discussed in application to the Sun and Galaxy.

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