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Observations of Large-Scale Dynamic Bubbles in Prominences

机译:突出中大规模动态泡沫的观察

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Solar prominences are very dynamic objects, showing continuous motions down to their smallest resolvable spatial and temporal scales. However, as macroscopic magnetic structures, they are remarkably stable during their quiescent phase. We present recent ground-based and Hinode observations of large-scale bubble-like, dynamic sub-structures that form within and rise through quiescent prominences without disrupting them. We investigate the similarities and differences of the Hinode and ground-based observations and discuss their implications for models of prominences.
机译:太阳能突出是非常动态的物体,显示出持续的动作到最小的可分辨空间和时间尺度。然而,作为宏观磁性结构,它们在静态阶段期间非常稳定。我们最近的基于地面和Hinode观察的大规模气泡状,动态子结构,在不扰乱它们的情况下通过静态突出来形成并升高。我们调查海线和基于地面观测的相似之处和差异,并讨论了对突出模式的影响。

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