Collaborative Research: GEM: Plasma Sheet Instabilities prior to THEMIS Substorm Expansion Onsets

合作研究：GEM：THEMIS 亚风暴扩张爆发之前的等离子体片不稳定性

• 批准号: 0902360
• 负责人: Ping Zhu
• 金额: $ 44万
• 依托单位: University of Wisconsin-Madison
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2009
• 资助国家: 美国
• 起止时间: 2009-09-01 至 2014-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0902360&HistoricalAwards=false
• 关键词: Collaborative; Research; GEM; Plasma; Sheet

This project contributes to the Geospace Environment Modeling (GEM) Focus Group on the early stages of the onset of a magnetospheric substorm. It will systematically analyze the plasma instabilities of the pre-onset, near-Earth plasmasheet substorm events. The plasma sheet conditions will be reconstructed using magnetohydrodynamic simulations with the OpenGGCM MHD code. Once the plasmasheet configuration is known, it will be possible to examine the stability of the configuration to macroscale instabilities such as ballooning, kink, and tearing modes. Both analytical eigenvalue methods and MHD simulations will be used in the stability analysis. The project will examine the signatures and consequences of the plasma instabilities and compare the results with observations made by the NASA THEMIS mission. The linear and early nonlinear instabilities of the plasmasheet during substorm growth phase are the keys to understanding the initial stage of the substorm expansion onset. The accuracy of the stability analyses relies on the detailed knowledge of the plasma sheet configuration model. THEMIS substorm observations will provide more input conditions and constraints that will enable the OpenGGCM simulation to reconstruct a sequence of accurate and realistic plasma sheet configurations during the substorm growth phase. The stability analysis will help resolve many remaining controversies on the onset process and bring in new perspectives on the substorm onset problem. The project will help provide quantitative interpretation of THEMIS substorm events, and will bridge the gap between theory, analysis and observations.

该项目为地球空间环境建模重点小组关于磁层亚暴开始的早期阶段作出了贡献。 它将系统地分析近地等离子体亚暴事件发生前的等离子体不稳定性。 等离子体片条件将使用磁流体动力学模拟与OpenGGCM MHD代码重建。 一旦等离子体的结构是已知的，它将有可能检查的宏观尺度不稳定性，如气球，扭结和撕裂模式的配置的稳定性。在稳定性分析中将使用解析特征值法和MHD模拟。该项目将研究等离子体不稳定性的特征和后果，并将结果与美国航天局THEMIS使命的观测结果进行比较。亚暴增长阶段等离子体的线性和早期非线性不稳定性是理解亚暴膨胀起始阶段的关键。稳定性分析的准确性依赖于等离子体片结构模型的详细知识。THEMIS亚暴观测将提供更多的输入条件和约束，使OpenGGCM模拟能够在亚暴生长阶段重建一系列准确和现实的等离子体片配置。稳定性分析将有助于解决许多剩余的争议的发病过程，并带来了新的角度亚暴发病问题。该项目将有助于提供THEMIS亚暴事件的定量解释，并将弥合理论、分析和观测之间的差距。