Acceleration of Radiation Belt Electrons: In Situ Heating vs. Inward Radial Transport

辐射带电子的加速：原位加热与向内径向传输

• 批准号: 0842388
• 负责人: Xinlin Li
• 金额: $ 30.23万
• 依托单位: University of Colorado at Boulder
• 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: 2009-04-01 至 2014-03-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0842388&HistoricalAwards=false
• 关键词: Acceleration; Radiation; Belt; Electrons; Situ

Electrons in Earth's radiation belts can have serious effects on spacecraft electronics through radiation damage and deep dielectric charging. The physical mechanisms governing the variability of these energetic electrons are still hot topics of debate. The paradigm for explaining the creation of the electron radiation belts has recently been shifting from one using only the theory of radial diffusion to one including an important role for plasma waves. The interaction of plasma waves with the electrons can result in in situ heating. This project will investigate the relative contribution of radial diffusion and in situ heating to the enhancement of MeV electrons inside geosynchronous orbit. An internal source term will be added to a currently existing radial diffusion model. Measurements of electrons using Los Alamos National Laboratory (LANL) satellite data at geosynchronous orbit will be used to determine the source population. Realistic loss rates will be determined from data taken from the SAMPEX satellite. The model results will then be compared to GPS satellite measurements inside geosynchronous orbit. In this way, it will be possible to determine how much enhancement of the MeV electrons measured by GPS can be attributed to inward radial transport and how much to in situ heating. This project will include research and training for graduate students. The results will enhance our ability to predict an important space weather phenomenon.

地球辐射带中的电子可能会通过辐射损伤和深层电介质充电对航天器电子设备产生严重影响。控制这些高能电子变化的物理机制仍然是争论的热门话题。解释电子辐射带形成的范式最近已经从仅使用径向扩散理论的范式转变为包括等离子体波的重要作用的范式。等离子体波与电子的相互作用可导致原位加热。该项目将研究径向扩散和原位加热对地球同步轨道内 MeV 电子增强的相对贡献。内部源项将添加到当前现有的径向扩散模型中。 使用洛斯阿拉莫斯国家实验室（LANL）在地球同步轨道上的卫星数据进行的电子测量将用于确定源群体。实际损失率将根据 SAMPEX 卫星获取的数据确定。然后将模型结果与地球同步轨道内的 GPS 卫星测量结果进行比较。通过这种方式，将有可能确定 GPS 测量到的 MeV 电子的增强有多少可归因于向内径向传输以及有多少可归因于原位加热。该项目将包括研究生的研究和培训。 研究结果将增强我们预测重要太空天气现象的能力。