在TRACERS任务上的Cusp Ions (ACI) 分析仪
Stephen A Fuselier1,2, Matthew A Freeman1, Craig A Kletzing3
1Southwest Research Institute, San Antonio, TX USA.
概括
在TRACERS任务上的Cusp离子分析仪 (ACI) 提供了地球磁层尖端离子速度分布函数的详细测量. 这些仪器可以精确检测尖端边界,并描述离子行为的特征.
科学领域:
- 空间物理 空间物理
- 磁层物理 磁层物理
- 等离子体物理学的物理学
背景情况:
- 磁层尖端是太阳风和地球磁层之间能量和粒子转移的关键区域.
- 了解尖端的离子动态对于理解太空天气现象和磁层过程至关重要.
研究的目的:
- 描述TRACERS任务上的Cusp Ions分析仪 (ACI) 仪器的能力.
- 突出ACI测量如何为TRACERS任务的科学目标提供贡献.
主要方法:
- 在旋转平台上使用圆形顶帽静电分析仪,以实现全角覆盖.
- 在低地球轨道上使用两个距离很近的航天器进行全面的数据采集.
- 测量离子速度分布功能具有高频率 (312 ms) 和良好的能量/角度分辨率.
主要成果:
- ACI仪器提供了一个广泛的离子能量范围 (∼8 eV/e到20,000 eV/e),有47个对数能量阶段.
- 实现分数能量分辨率≤10%和即时角分辨率为22.5° × ∼6°.
- 展示检测尖端边界的能力,并以灵敏和精确的态度描述离子步骤.
结论:
- ACI非常适合在磁层尖端对离子行为进行详细的现场测量.
- 这些测量对于我们进一步了解尖端过程及其对太空天气的影响至关重要.
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