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电子加速在范艾伦辐射带的中心
G D Reeves1, H E Spence, M G Henderson
1Space Science and Applications Group, Los Alamos National Laboratory, Los Alamos, NM 87545, USA. reeves@lanl.gov
概括
科学家们发现了超相对论电子如何在地球的范·艾伦辐射带中获得高能量. 测量显示皮带内的局部加速度,而不是来自外部来源的,是主要的机制.
科学领域:
- * 空间物理学和等离子体物理学
- * 地球磁层的动力学
- * 粒子加速机制 粒子加速机制
背景情况:
- * 范·艾伦辐射带含有超相对论电子,构成了持续的科学.
- * 存在两个主要假设:来自外部源的辐射加速或带内的局部加速.
- * 了解电子加速对于太空天气预测和卫星安全至关重要.
研究的目的:
- * 为了区分范艾伦带电子的辐射和局部加速机制.
- * 为主导电子加速过程提供了明确的证据.
主要方法:
- *利用了美国宇航局的范艾伦辐射带风暴探测器 (RBSP) 的数据.
- *分析了电子相位空间密度的辐射形状.
- * 将观测数据与理论加速模型进行比较.
主要成果:
- *观察到的相空间密度概况强烈支持局部加速.
- *数据与主要的辐射加速过程不一致.
- * 直接区分两种拟议的加速机制.
结论:
- * 范·艾伦辐射带内的局部加速度是激活电子的主要机制.
- *来自外部源的辐射传输在高能电子加速中起到较小的作用.
- *这些发现解决了磁层物理学中长期存在的问题.
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