探测器观测了水星的电离系外层和等离子环境的组成
Thomas H Zurbuchen1, Jim M Raines, George Gloeckler
1Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109-2143, USA. thomasz@umich.edu
概括
水星 水星 水星 水星 水星
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:
- 水星的太空环境充满了来自太阳风相互作用和外层电离的离子.
- 以前的观测表明,在水星的外层中存在 (Na+),氧 (O+) 和 (K+) 离子.
研究的目的:
- 用MESSENGER数据分析水星磁层中离子的组成和分布.
- 为了研究水星的等离子环境中的离子的起源和能量.
主要方法:
- 来自MESSENGER航天器观测的离子丰度和流量的分析.
- 解释每电荷质量 (m/q) 的光谱数据以识别离子物种.
主要成果:
- 检测硫 (S+) 和硫化 (H2S+) 离子,其中 (S+ + H2S+) / (Na+ + Mg+) = 0.67 +/- 0.06.
- 在m/q=18的水基离子的鉴定,与Na+加Mg+相比,其度为0.20 +/- 0.03.
- 观察到由衍生的离子,包括更重的物种,填满了磁层.
结论:
- 存在S +,H2S +和水组离子,扩大了我们对水星外层构成的理解.
- 双重电离的物种表明在水星的磁层内有显著的电子能量 (<1 keV).
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