Magnetic Reconnection in Solar Flares

这项已完成的基于更新的提案要求提供两年的资金，以继续与太阳耀斑中的磁场重联有关的研究。之前开发的计算机代码现在将用于研究双带耀斑、日冕物质抛射和日冕物质抛射。该模型显示了对所有这些现象进行研究并得出关于它们的起源和特征的具体结果的希望。将大力考虑与现有观测数据有关的问题。***

This accomplished based renewal proposal requests funds for two years to continue research related to magnetic reconnection in solar flares. The previously developed computer code will now be employed to study two-ribbon flares, prominence disruptions, and coronal mass ejections. The model shows promise for investigating all of these phenomena and arriving at specific results concerning their origin and characteristics. A strong effort will be made to consider problems which relate to existing observational data. ***