Linking the solar chromosphere and corona: IRIS and AIA/SDO observations of dynamic events

该项目将开发各种方法，以便在IRIS对太阳色球层（低层大气）的观测中自动探测和分类明亮的动态事件，并寻求与AIA/SDO观测到的日冕（高层大气）变化之间的统计关系。连接这些大气层是理解将日冕加热到一百万度以上的过程的关键一步。该项目还将包括由瑞典太阳望远镜等望远镜进行的地面测量。

This project will develop methods to automatically detect and categorize bright dynamic events in IRIS observations of the solar chromosphere (the lower atmosphere), and to seek statistical relationships with changes in the corona (the higher atmosphere) observed by AIA/SDO. Connecting these atmospheric layers is a critical step towards understanding the processes that heat the solar corona to over a million degrees. This project will also incorporate ground-based measurements made by telescopes such as the Swedish Solar Telescope (SST).