通量涌现(理论)

IF 20.9 1区物理与天体物理

Living Reviews in Solar Physics Pub Date : 2014-07-17 DOI:10.12942/lrsp-2014-3

Mark C. M. Cheung, Hiroaki Isobe

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引用次数: 151

摘要

从太阳对流区进入上覆大气的磁通量是一系列与太阳活动有关的现象的驱动因素。在这篇文章中，我们介绍了磁涌现研究的核心理论概念，并讨论了在模型中包含不同的物理效应(例如，磁浮力、磁对流、重联、磁扭曲、与环境场的相互作用)如何影响新兴场和等离子体的演变。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

Flux Emergence (Theory)

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Flux Emergence (Theory)

Magnetic flux emergence from the solar convection zone into the overlying atmosphere is the driver of a diverse range of phenomena associated with solar activity. In this article, we introduce theoretical concepts central to the study of flux emergence and discuss how the inclusion of different physical effects (e.g., magnetic buoyancy, magnetoconvection, reconnection, magnetic twist, interaction with ambient field) in models impact the evolution of the emerging field and plasma.

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来源期刊

Living Reviews in Solar Physics ASTRONOMY & ASTROPHYSICS-

自引率

1.40%

发文量

期刊介绍： Living Reviews in Solar Physics, a platinum open-access journal, publishes invited reviews covering research across all areas of solar and heliospheric physics. It distinguishes itself by maintaining a collection of high-quality reviews regularly updated by the authors. Established in 2004, it was founded by the Max Planck Institute for Solar System Research (MPS). "Living Reviews®" is a registered trademark of Springer International Publishing AG.