色球耀斑
Chromospheric Flares
摘要：
在这篇专题评论中，我重新审视了“色球耀斑”。“这目前应该是一个过时的概念，因为现代数据似乎排除了单独在色球层中发生重大耀斑的可能性，但色球层仍然在许多方面发挥着重要的观测作用。它是耀斑辐射能量的主要来源-特别是可见光/紫外线连续辐射。它还提供了示踪剂，引导我们找到能量的日冕源，尽管我们还不了解能量从日冕中的储存到色球层中的释放的传播过程。耀斑期间色球辐射的形成提出了几个困难而有趣的物理问题。
英文摘要：
In this topical review I revisit the "chromospheric flare." This should currently be an outdated concept, because modern data seem to rule out the possiblity of a major flare happening independently in the chromosphere alone, but the chromosphere still plays a major observational role in many ways. It is the source of the bulk of a flare's radiant energy - in particular the visible/UV continuum radiation. It also provides tracers that guide us to the coronal source of the energy, even though we do not yet understand the propagation of the energy from its storage in the corona to its release in the chromosphere. The formation of chromospheric radiations during a flare presents several difficult and interesting physical problems.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
