Living Reviews in Solar Physics ( IF 23.0 ) Pub Date : 2018-10-22 , DOI: 10.1007/s41116-018-0016-2 Sarah E Gibson 1
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Magnetic fields suspend the relatively cool material of solar prominences in an otherwise hot corona. A comprehensive understanding of solar prominences ultimately requires complex and dynamic models, constrained and validated by observations spanning the solar atmosphere. We obtain the core of this understanding from observations that give us information about the structure of the “magnetic skeleton” that supports and surrounds the prominence. Energetically-sophisticated magnetohydrodynamic simulations then add flesh and blood to the skeleton, demonstrating how a thermally varying plasma may pulse through to form the prominence, and how the plasma and magnetic fields dynamically interact.
中文翻译：
日珥：理论和模型
磁场将太阳日珥中相对较冷的物质悬浮在炽热的日冕中。对太阳日珥的全面了解最终需要复杂的动态模型，并通过跨越太阳大气层的观测进行约束和验证。我们从观察中获得了这种理解的核心，这些观察为我们提供了有关支撑和围绕日珥的“磁骨架”结构的信息。然后，能量复杂的磁流体动力学模拟将血肉添加到骨骼中，演示热变化等离子体如何脉冲通过以形成突出物，以及等离子体和磁场如何动态相互作用。
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