Dynamics of the Inner Radiation Belt Near the Trapping Limit

接近俘获极限的内辐射带动力学

• 批准号: 1023332
• 负责人: Mary Hudson
• 金额: $ 30万
• 依托单位: Dartmouth College
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2011
• 资助国家: 美国
• 起止时间: 2011-07-15 至 2015-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1023332&HistoricalAwards=false
• 关键词: Dynamics; Inner; Radiation; Belt; Near

This project will undertake a systematic study of the complex particle dynamics of Earth's innder radiation belt. It will determine the quantitative effects of several different phenomena that can affect the radiation belt proton content. The principal tool in this work will be numerical integration of the dynamical equations to determine proton paths in model magnetospheric fields. Satellite data show significant losses of ~10 MeV radiation belt protons from the inner radiation belt during magnetic storms. These observations will provide stringent tests of the results obtained from the modeling work. Simplified magnetic field models will be used to which effects are most significant. Then detailed magnetospheric models will be used to calculate realistic results. The models will be tested by comparison with observed geomagnetic cutoff variations. Induced electric fields, which are important for both radial transport and particle acceleration, will be determined by application of Faraday?s law in the time dependent magnetic field models. Injections of solar energetic protons (SEPs) into the radiation belt are a significant source of trapped protons and have also been extensively characterized by satellite measurements. Cutoff suppression during magnetic storms provides solar proton access to the trapping region. Whether this can lead to permanent trapping will be assessed by reversing the numerical simulations of storm-time losses to determine if the protons originated in the untrapped solar protons.This project addresses an important question concerning the dynamics of the inner radiation belt. Energetic particles in the inner radiation belt are a significant hazard to satellites that pass through the belt. Solar energetic protons are one of the most important hazards affecting spacecraft operations. In addition to the relevance of the project to our understanding of an important space weather phenomenon, the project has a strong educational component with much of the research being carried out by a graduate student.

该项目将对地球内部辐射带的复杂粒子动力学进行系统研究。 它将确定可能影响辐射带质子含量的几种不同现象的定量效应。这项工作的主要工具将是动力学方程的数值积分，以确定质子在模型磁层场中的路径。卫星数据显示，在磁暴期间，来自内辐射带的~10 MeV辐射带质子大量丢失。 这些观测结果将为从建模工作中获得的结果提供严格的检验。简化的磁场模型将被用于哪些影响是最显着的。然后，详细的磁层模型将用于计算现实的结果。将通过与观测到的地磁截止变化进行比较来检验这些模型。感应电场，这是很重要的径向运输和粒子加速，将通过应用法拉第？s定律在含时磁场模型中的应用。太阳高能质子（SEPs）注入辐射带是捕获质子的重要来源，并且也已通过卫星测量进行了广泛的表征。磁暴期间的截止抑制提供了太阳质子进入捕获区域的机会。这是否会导致永久性的捕获，将通过逆转风暴时间损失的数值模拟来评估，以确定质子是否起源于未捕获的太阳质子。 内辐射带中的高能粒子对通过该带的卫星是一个重大危险。 太阳高能质子是影响航天器运行的最重要危险之一。 除了该项目与我们对一种重要的空间气象现象的认识有关外，该项目还具有很强的教育成分，其中许多研究是由一名研究生进行的。