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...

詳細記述

書誌詳細
主要な著者: Schekochihin, A, Cowley, S, Maron, J, Malyshkin, L
フォーマット: Journal article
言語:English
出版事項: 2002

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