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.

中文翻译：

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通量出现（理论）

从太阳对流区进入上层大气的磁通量是与太阳活动相关的各种现象的驱动因素。在本文中，我们介绍了通量出现研究的核心理论概念，并讨论了模型中包含的不同物理效应（例如磁浮力、磁对流、重联、磁扭曲、与环境场的相互作用）如何影响新兴通量的演化。场和等离子体。