Mirror Asymmetry and Helicity Invariants in Astrophysical Dynamos


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

The mirror asymmetry of hydrodynamics flows and magnetic fields plays a crucial role in magnetic field evolution in various celestial bodies including the Earth, Sun and Milky Way galaxy. A natural measure of the mirror asymmetry is associated with the Gauss invariant, i.e. the linkage number of vortex and magnetic lines. We consider the relation between magnetic field generation and the knotting of vortex and magnetic lines in terms of hydrodynamic and magnetic helicities. Higher helicity invariants known in topology generalize in various ways the Gauss invariant. We argue that these higher helicities are less important for magnetic field evolution than the classical Gauss invariant.

作者简介

D. Sokoloff

Department of Physics, Moscow State University; IZMIRAN

编辑信件的主要联系方式.
Email: sokoloff.dd@gmail.com
俄罗斯联邦, Moscow, 119991; TroitskMoscow, 108840

补充文件

附件文件
动作
1. JATS XML

版权所有 © Pleiades Publishing, Ltd., 2019