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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
在木星附近的等离子观测:旅行者2号的初步结果
概括
旅行者2号旅行者2号
科学领域:
- 行星科学 行星科学
- 空间物理 空间物理
- 等离子体物理学的物理学
背景情况:
- 旅行者2号的入境通道提供了关于木星磁层的关键数据.
- 旅行者1号先前的观测已经确定了基线血特性.
研究的目的:
- 详细介绍旅行者2号的磁层穿越和等离子体观测.
- 分析木星磁层中的等离子体行为,组成和结构.
主要方法:
- 旅行者2号在现场测量了等离子体密度,强度和组成.
- 分析行星旋转调制以推断等离子体板的几何形状.
主要成果:
- 多个弓冲击穿越和磁层进入在特定的木星半径.
- 等离子体呈现出角化;密度和强度与旅行者1号相美.
- 由重离子主导的磁层等离子体 (质量密度比~100:1).
- 在甘尼米德附近观察到等离子体强度下降,表明复杂的相互作用.
- 最初以双极赤道为中心的等离子板,随着距离的增加,向旋转赤道偏离.
- 等离子板的纵向位置落后于旋转的双极.
结论:
- 旅行者2号的数据证实并扩展了关于木星磁层的先前发现.
- 磁层的结构和动力学受到重离子和与甘尼米德等卫星的相互作用的影响.
- 等离子板的复杂几何和行为为木星磁层过程提供了洞察力.
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