Observations of Solar Active Region Current System and Solar Flares During MAX'91 and Solar-A

PI申请资金以运行新的成像向量 米斯太阳天文台在高太阳活动期间的地磁仪 太阳活动，以支持马克斯'91运动， 个人研究项目。 他个人的目标 研究项目包括： (1)从光球矢量磁图中确定 耀斑活动区日冕磁场 不仅是非潜在的，也是非力的， 自由，并了解这种偏离的起源; (2)了解光球的形态关系 磁场和电流系统， 非热电子加速和沉淀 照明弹; (3)为了确定Ho极化的时间依赖性， 在耀斑期间，并了解其与 高能质子在我们不太了解的亚兆电子伏范围内。 ***

The PI request funds to operate the new Imaging Vector Magnetograph at Mees Solar Observatory during the period of high solar activity, in support of both Max '91 campaigns and individual research projects. The goals of his individual research projects include: (1) to determine from photospheric vector magnetograms whether coronal magnetic fields in flare-productive active regions are demonstrably not only non-potential, but also non-force- free, and to understand the origin of such departures; (2) to understand the morphological relationship of photospheric magnetic fields and current systems to bulk energization and nonthermal electron acceleration and precipitation in flares; (3) to determine the temporal dependence of Ho polarization during flares, and to understand its relationship to energetic protons in the ill-understood sub-Mev range. ***