High Resolution Observations of Evolution of Magnetic Fields and Flows Associated with Solar Eruptions

这个为期3年的项目旨在研究与太阳耀斑相关的磁场演化，这有望揭示导致太阳喷发的潜在物理机制(S)-空间天气的主要驱动因素。该项目有很强的教育成分：它将主要支持一名女性研究生以及一名女性初级研究员。该项目将产生的数据分析和图像处理工具可用于科学和工程的许多其他领域。该项目的研究和EPO议程支持AGS部门在发现、学习、多样性和跨学科研究方面的战略目标。这个为期3年的项目的主要目的是研究与太阳喷发相关的矢量磁场和流动运动的演变。该项目的具体科学目标是：(I)增进对太阳喷发后光球磁场快速变化的物理了解，(Ii)研究与这些喷发有关的光球水平和垂直流动运动。项目团队将使用最新的最新数据以及来自SDO和NST的持续新观测。进行研究研究所需的大多数数据分析工具都是由项目组在过去开发和验证的。

This 3-year project is aimed at studying the solar-flare-associated magnetic field evolution, which has the promise to reveal the underlying physical mechanism(s) responsible for solar eruptions --- the main drivers of space weather. The project has a strong education component: it will mainly support a female graduate student as well as a female junior researcher. The data analysis and imaging processing tools that will result from this project can be used in many other areas of science and engineering. The research and EPO agenda of this project supports the Strategic Goals of the AGS Division in discovery, learning, diversity, and interdisciplinary research. The main thrust of this 3-year project is to investigate the evolution of vector magnetic fields and flow motions associated with solar eruptions. The specific science objectives of the project are to (i) gain improved physical understanding of the rapid changes of photospheric magnetic fields following solar eruptions, and (ii) study the photospheric flow motions, both horizontal and vertical, associated with these eruptions. The project team will use recent state-of-the-art data as well as continuing new observations from SDO and NST. Most of the data analysis tools that are needed to conduct the research studies have been developed and validated by the project team in the past.