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

与太阳喷发相关的磁场和气流演化的高分辨率观测

• 批准号: 1408703
• 负责人: Haimin Wang
• 金额: $ 39.64万
• 依托单位: New Jersey Institute of Technology
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2014
• 资助国家: 美国
• 起止时间: 2014-09-01 至 2019-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1408703&HistoricalAwards=false
• 关键词: Resolution; Observations; Evolution; Magnetic; Fields

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.

这个为期三年的项目旨在研究太阳能相关的磁场演化，该磁场的演变有望揭示负责太阳喷发的潜在物理机制 - 这是太空天气的主要驱动因素。 该项目具有强大的教育部分：它将主要支持女研究生以及女性初级研究员。 该项目将导致的数据分析和成像处理工具可以用于许多其他科学和工程领域。 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。这个三年项目的主要目的是研究与太阳喷发相关的向量磁场和流动运动的演变。 该项目的特定科学目标是（i）提高对太阳喷发后光电磁场快速变化的物理理解，以及（ii）研究与这些喷发相关的水平和垂直方向的光球流动运动。 项目团队将使用最新的最新数据，并继续从SDO和NST进行新的观察结果。 过去，项目团队已经开发和验证了进行研究研究所需的大多数数据分析工具。