Magnetic Reconnection in Solar Flares

这一已完成的更新提案要求提供资金， 用两年时间继续研究磁场重联 在太阳耀斑中。 以前开发的计算机代码现在将 可以用来研究双带耀斑、日珥破裂、 和日冕物质抛射该模型显示了 调查所有这些现象， 关于其起源和特征的研究结果。一个强大 将努力考虑与现有的 观测数据***

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. ***