相关实验视频
Updated: Jul 12, 2026

06:53
Photoelectron Imaging of Anions Illustrated by 310 Nm Detachment of F−
Published on: July 27, 2018
概括
宇宙射线观测显示,木星内部有充满活力的硫,和氧核.
科学领域:
- 行星科学 行星科学
- 空间物理 空间物理
- 天体物理学 天体物理学
背景情况:
- 木星的磁层是一个复杂的区域,受到太阳风和内部过程的影响.
- 以前对木星磁层的了解是有限的,特别是关于能量粒子的组成和分布.
研究的目的:
- 为了研究木星磁层内的能量粒子的组成和分布.
- 为了描述磁层尾部和能量质子增强的特征.
主要方法:
- 利用宇宙射线子系统进行现场观测.
- 分析了粒子能量,组成和空间分布.
主要成果:
- 在Io的轨道内发现了充满活力的硫,和氧核 (>7 MeV/核子).
- 在11个木星半径之外的磁层中观察到类似太阳宇宙射线的离子.
- 在木星活跃半球中发现30-70%的能量质子增强.
- 首次观察到磁层尾部延伸到木星半径160度的黎明方向.
结论:
- 木星的磁层含有意想不到的能量离子群,包括重元素.
- 太阳能粒子的影响延伸到木星磁层的深处.
- 能量粒子动力学受到木星的旋转和磁层活动的重大影响.
- 磁层尾巴比以前理解的更为广泛.
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