一个磁性签名在Io:利略磁力计的初步报告
1M. G. Kivelson, K. K. Khurana, R. J. Walker, C. T. Russell, Institute of Geophysics and Planetary Physics, University of California, Los Angeles, Los Angeles, CA 90095-1567, USA. J. A. Linker, Science Applications International Corporation, San Diego, CA 92171, USA. D. J. Southwood, Department of Physics, Imperial College of Science, Technology, and Medicine, London, SW7 2BZ, UK. C. Polanskey, Jet Propulsion Laboratory, Pasadena, CA 91109, USA.
概括
利略航天器的数据表明,木星的卫星Io拥有自己的内在磁场. 这种由动力发电机作用产生的内在电场是对在Io附近观察到的磁场扰动的最合理的解释.
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:
- 木星的卫星Io以其强烈的火山活动和与木星磁层的相互作用而闻名.
- 以前的研究已经讨论了在Io附近观察到的磁场异常的来源.
- 了解Io的内部结构和磁性质对于行星形成理论至关重要.
研究的目的:
- 为了调查在利略航天器在Io的飞越过程中观察到的磁场扰动的来源.
- 要确定等离子体相互作用还是内在磁场最能解释数据.
- 评估Io拥有全球内在磁场的可能性.
主要方法:
- 通过利略航天器磁力计获得的1分钟平均磁场测量的分析.
- 将观察到的现场数据与基于等离子体源和诱导磁场的模型进行比较.
- 对与动力发电机理论相一致的内在磁场假设的评估.
主要成果:
- 在Io附近记录了木星磁场的显著下降 (近40%).
- 仅仅是等离子体来源无法解释观测到的磁扰动的大小.
- 一个诱导的磁场需要在Io的地幔中不切实际地高度的铁.
结论:
- 观测到的磁场数据强烈支持了由Io产生的内在磁场的假设.
- 在Io内部的动力发电机被提出为产生这种内在场的机制.
- 伊奥可能是一个磁化固体行星,类似于地球和水星.
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