Structure of small-scale magnetic fields in the kinematic dynamo theory.

Structure of small-scale magnetic fields in the kinematic dynamo theory.

A weak fluctuating magnetic field embedded into a a turbulent conducting medium grows exponentially while its characteristic scale decays. In the interstellar medium and protogalactic plasmas, the magnetic Prandtl number is very large, so a broad spectrum of growing magnetic fluctuations is excited...

Szczegółowa specyfikacja

Opis bibliograficzny
Główni autorzy:	Schekochihin, A, Cowley, S, Maron, J, Malyshkin, L
Format:	Journal article
Język:	English
Wydane:	2002

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