欧洲的磁性签名:从1996年12月19日的利略通行证报告
M G Kivelson1, K K Khurana, S Joy
1Institute of Geophysics and Planetary Physics and Department of Earth and Space Sciences, University of California, Los Angeles, Los Angeles, CA 90095-1567, USA.
概括
利略航天器的数据表明,木星的卫星欧罗巴可能具有内部磁场,磁场干扰证明了这一点. 然而,这个内部场没有得到证实,它的方向是不寻常的.
科学领域:
- 行星科学 行星科学
- 磁动力学 磁动力学
- 地质物理学 地质物理学
背景情况:
- 木星的卫星欧罗巴拥有微薄的大气层,与木星强大的磁层相互作用.
- 之前的任务提供了关于欧罗巴固有的磁性特性有限的数据.
研究的目的:
- 为了调查由利略航天器在欧洲附近观测到的磁场扰动的来源.
- 确定欧罗巴是否具有内在磁场,并描述其特性.
主要方法:
- 1996年12月19日,利略航天器在欧洲的近距离飞行中对磁力计数据的分析.
- 模拟磁场扰动,以测试内部欧罗巴双极场和外部等离子体电流的假设.
主要成果:
- 观测到的磁场扰动与木星的背景磁场有很大差异.
- 数据与以欧罗巴为中心的二极子时刻一致,高达大约240纳米级,表明潜在的内部场.
- 双极方向与欧罗巴的旋转轴和木星强加的场相比是斜的,这对于动力发电机产生的场来说是不寻常的.
- 在欧罗巴附近的小规模扰动表明局部等离子体电流的影响.
结论:
- 虽然数据可以用内部欧罗巴双极场来建模,但其存在尚未得到证实.
- 潜在双极的斜方向不易通过核心动力发电机机制来解释.
- 等离子体电流可能有助于欧洲附近的小规模磁场变化.
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