概括
旅行者2号在土星中检测到更强烈和更可变的宇宙射线质子和电子流.
科学领域:
- 行星科学 行星科学
- 磁层物理 磁层物理
- 宇宙射线物理学 宇宙射线物理学
背景情况:
- 旅行者2号提供了土星磁层的现场测量.
- 之前的观测确定了土星磁层的基线条件.
研究的目的:
- 为了展示旅行者2号上的宇宙射线系统的结果.
- 分析粒子流量变化及其原因.
- 通过使用卫星吸收特征来约束土星的内部磁极.
主要方法:
- 来自旅行者2号的宇宙射线系统数据的分析.
- 观测土星磁层中的质子和电子流.
- 使用Mimas,Enceladus和Tethys的带电粒子吸收签名.
主要成果:
- 增加的质子流量 (>0.43 MeV) 和更大的变化在进口通道期间的质子和电子流.
- 在18个土星半径之外观测到的冲动性电子爆炸 (0.14-1.0 MeV)
- 过渡性电子流量减少在3个土星半径附近,不能归因于Mimas,这表明了额外的材料.
结论:
- 观察到的粒子流量变化归因于太阳风的变化.
- 卫星的吸收信号限制了土星的磁二极点倾斜和偏移.
- 有证据表明,Mimas轨道上存在未经证实的物质或卫星.
相关概念视频
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