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The True Relationship between "Precursor" Phenomena, Magnetic Topology, and Solar Energetic Events

“前驱”现象、磁拓扑和太阳高能事件之间的真实关系

基本信息

批准号：
2154653
负责人：
Karin Dissauer
金额：
$ 74.74万
依托单位：
NorthWest Research Associates, Incorporated
依托单位国家：
美国
项目类别：
Standard Grant
财政年份：
2022
资助国家：
美国
起止时间：
2022-04-01 至 2025-03-31
项目状态：
未结题

来源：
https://www.nsf.gov/awardsearch/showAward?AWD_ID=2154653&HistoricalAwards=false
关键词：
True Relationship between Precursor Phenomena

项目摘要

Small-scale changes occur on the Sun prior to the onset of powerful and impactful events like solar flares and coronal mass ejections (CMEs). These changes are known as a “precursor” and indicate processes occurring that may trigger the larger energetic events. This project investigates precursor events to determine which can lead to these impactful events. Powerful solar flares and CMEs create major space weather impacts that cause diverse effects for human technology, including damage to satellites and power grid systems. The broader impacts of the project include understanding these important natural phenomena, training undergraduate students, supporting an early career researcher, and creation of tutorials for the public on science topics. The science goal of the project is to establish the uniqueness and causal relationship of precursor transient activity to solar flares and CMEs in order to better understand magnetic reconnection and the subsequent initiation of solar energetic events. The objectives to meet this goal are (1) quantify the differences in temporal, spatial, and physical characteristics of precursors against similar phenomena during activity-quiet epochs, thus solidifying a statistical association and identifying physical uniqueness, and (2) investigate the magnetic connection between precursors and a subsequent event’s energy release and eruption dynamics, thus solidifying a causal relationship. To achieve these objectives the researchers will analyze ~1000 events and matched event-quiet controls (both flare-quiet epochs and CME-less flare events) in coordination with a newly-funded NASA effort (HGI#80NSSC21K0738). The pre-event signatures’ temporal behavior, photospheric magnetic context, coronal dynamics, temperature and density will be investigated using high-order moment analysis of their photospheric vector magnetic field and extreme ultraviolet (EUV) emission applying Differential Emission Measure (DEM) analysis. Established statistical classifier codes and Bayesian counting statistics will be used to evaluate the differences between flare/CME-related precursors and transients from activity-quiet controls. Magnetic association between pre-event brightenings and dimmings and the initial flare/eruption site will be established using Magnetic Charge Topology (MCT) analysis, validated by nonlinear force-free coronal models.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

在太阳耀斑和日冕物质抛射（CME）等强大而有影响力的事件发生之前，太阳会发生小规模的变化。这些变化被称为“前兆”，表明可能引发更大能量事件的过程。该项目调查前兆事件，以确定哪些可能导致这些有影响力的事件。强大的太阳耀斑和日冕物质抛射会产生重大的空间天气影响，对人类技术造成各种影响，包括对卫星和电网系统的破坏。该项目更广泛的影响包括了解这些重要的自然现象，培训本科生，支持早期职业研究人员，并为公众创建科学主题的教程。该项目的科学目标是确定太阳耀斑和日冕物质抛射的前兆瞬变活动的独特性和因果关系，以便更好地了解磁场重联和随后引发的太阳高能事件。实现这一目标的目标是：（1）量化活动-平静时期前兆与类似现象在时间、空间和物理特征上的差异，从而巩固统计关联并确定物理独特性;（2）调查前兆与后续事件的能量释放和喷发动力学之间的磁性联系，从而巩固因果关系。为了实现这些目标，研究人员将分析约1000个事件和匹配的事件安静控制（包括耀斑安静时期和CME无耀斑事件），并与新资助的NASA工作（HGI#80NSSC21K0738）协调。将利用对光球矢量磁场的高阶矩分析和应用差分发射测量分析的极紫外线发射来研究事件前特征的时间行为、光球磁背景、日冕动力学、温度和密度。已建立的统计分类器代码和贝叶斯计数统计将用于评估耀斑/日冕物质抛射相关前兆和活动-安静对照瞬变之间的差异。事件前的增亮和变暗与初始耀斑/喷发地点之间的磁关联将通过磁荷拓扑（MCT）分析建立，并通过非线性无力日冕模型进行验证。该奖项反映了NSF的法定使命，并通过使用基金会的知识价值和更广泛的影响审查标准进行评估，被认为值得支持。