Imaging Microwave Spectroscopy of the Sun with the Owens Valley Solar Array

这项研究将分析已经观测到的数百个耀斑事件，以及随着太阳活动增加而即将发生的其他事件。 耀斑工作将测量大量事件的单个或多个耀斑源中的等离子体参数，如电子空间和能量分布、磁场强度和环境密度。 PI将使用新的空间/光谱MEM算法从当前和未来的突发数据中获得改进的快照图像，从而获得改进的光谱，从中提取这些物理参数。 此外，他将研究活跃地区，因为他们在磁盘上旋转，采用技术，如立体视觉和空间/光谱MEM重建，可能会给稳定的活跃地区的高度结构，从不同的角度来看，太阳旋转。

This research will analyze hundreds of flare events already observed, as well as additional events yet to come as solar activity increases. The flare work will measure plasma parameters such as electron spatial and energy distributions, magnetic field strength, and ambient density in single or multiple flare sources for a large number of events. The PI will obtained improved snapshot images from both current and future burst data using a new spatial/spectral MEM algorithm, hence obtaining improved spectra from which to extract these physical parameters. In addition, he will study active regions as they rotate across the disk, employing techniques such as stereoscopy and the spatial/spectral MEM reconstruction, potentially giving the height structure of stable active regions viewed from different aspect angles as the Sun rotates.