来自MESSENGER轨道观测的水星全球磁场
Brian J Anderson1, Catherine L Johnson, Haje Korth
1The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA. brian.anderson@jhuapl.edu
概括
水星的磁场从它的旋转轴向北偏移,磁轴倾斜. 这种内部磁场最好用一个偏移二极体来表示,其行星时刻为195 ± 10nT·R (M) 3.
科学领域:
- 行星科学 行星科学
- 地质物理学 地质物理学
- 空间物理 空间物理
背景情况:
- 水星拥有全球磁场,这对于陆地行星来说是一个罕见的特征.
- 了解水星的磁场对于理解它的内部动力发电机和太空环境至关重要.
研究的目的:
- 使用MESSENGER航天器数据来描述水星的内部磁场.
- 为了确定水星磁双极的偏移和方向.
- 为了量化行星的磁矩.
主要方法:
- 从磁计数据中分离内部和外部磁场贡献.
- 将内部场建模为一个自旋对齐的偏移双极.
- 通过识别辐射磁场组件中的零点来绘制磁赤道的地图.
- 使用磁断层交叉来定义一个外部场模型.
主要成果:
- 磁赤道偏移在地理赤道以北484±11公里处.
- 水星的磁轴与其旋转轴相比倾斜不到3°.
- 最适合的行星磁矩是195 ± 10纳米斯拉-R (M) 3.
结论:
- 水星的内部磁场最好用偏移双极模型来描述.
- 北方偏移和轻微倾斜提供了对地球动力发电机过程的洞察.
- 探测器的数据显著提高了我们对水星内在磁场的理解.
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