水星磁场的结构来自MESSENGER首次飞越的磁场
Brian J Anderson1, Mario H Acuña, Haje Korth
1Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA. brian.anderson@jhuapl.edu
概括
探测器MESSENGER证实了水星近赤道的磁场强度与Mariner 10的发现相似. 分析表明,该场可能是纯粹的中心二极体,尽管更高阶的组件也是可能的.
科学领域:
- 行星科学 行星科学
- 磁动力学 磁动力学
- 空间物理 空间物理
背景情况:
- 水星拥有全球磁场,这对于理解它的内部动力学至关重要.
- 玛丽纳10号之前的测量提供了关于水星赤道磁场的初始数据.
研究的目的:
- 为了展示来自MESSENGER第一个水星飞越的磁场测量.
- 描述水星近赤道磁场,并将其与之前的观测结果进行比较.
主要方法:
- 分析了MESSENGER航天器在其首次飞越期间收集的磁场数据.
- 使用中心双极和多极解决方案对磁场进行建模.
主要成果:
- 探测器的测量显示,场强度与Mariner 10的赤道数据保持在10%的范围内.
- 二极解决方案表明一个向南的行星时刻在230-290 nT·RM3之间,与旋转轴倾斜5°-12°.
- 多极解决方案揭示了双极场大小的22%至52%的非双极贡献.
结论:
- 观测到的磁场与纯中心双极和具有显著更高阶组件的磁场一致.
- 磁断,尾流和等离子体压力效应可能有助于观察到的磁场复杂性.
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