在太阳南极上方:低能量的行星间带电粒子
L J Lanzerotti1, T P Armstrong, R E Gold
1AT&T Bell Laboratories, Murray Hill, NJ 07974, USA.
概括
天球电流板显著塑造了日球,甚至在极地地区. 星际冲击加速了远离尤利西斯的电子.
科学领域:
- 太空物理空间物理学
- 太空物理学 太空物理学
- 血物理学的等离子体物理学
背景情况:
- 日球的结构受到太阳活动和磁场的影响.
- 了解日球中的粒子运输对于太空天气预测至关重要.
研究的目的:
- 为了研究日球流表对南极地区粒子流量的影响.
- 分析低能离子和电子的加速机制.
主要方法:
- 利用了来自Ulysses航天器上的光谱,组成和异位变异仪 (HISCALE) 的日球仪器的数据.
- 在极地交叉过程中分析了低能离子和电子 (> 50 keV) 的流量.
主要成果:
- 日球电流板显著影响了日球的结构,直到-75度的日.
- 星际反射冲击加速了远离乌利塞斯航天器的电子.
- 异常的氧气流量和Ne/O比率在高度度处测量.
结论:
- 日球电流板在塑造日球方面发挥着主导作用.
- 粒子加速与电流板动力学和行星间冲击有关.
- 需要进一步的研究来澄清在更高的度度处低能电子流量增强的情况.
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