木星磁层的黄昏侧面是木星磁层的黄昏侧面
W S Kurth1, D A Gurnett, G B Hospodarsky
1Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa 52242, USA. william-kurth@uiowa.edu
Nature
|March 5, 2002
概括
木星的磁断层随着太阳风的压力而缩小和膨胀,类似于地球的磁断层. 这项研究使用两点测量来证实这种行为,并发现了木星磁断层内的边界层的证据.
科学领域:
- 行星科学 行星科学
- 空间物理 空间物理
- 磁层物理 磁层物理
背景情况:
- 木星的磁断动态以前是从有限的单一航天器数据推断出来的.
- 地球的磁断层运动是使用多个航天器观测的充分研究.
研究的目的:
- 为了研究木星对太阳风压力变化的磁断反应.
- 为了比较木星磁断的行为与地球磁层.
主要方法:
- 利用几乎同时对木星磁断的两点测量.
- 在从更大到更小的磁断尺寸过渡期间分析数据.
主要成果:
- 木星的磁断层在应对太阳风压力变化时表现出类似的向内/向外运动,就像地球的磁断层一样.
- 证实了地球磁层物理学对木星的有效性.
- 观察到的证据表明磁断层内部有一个发达的边界层.
结论:
- 木星对太阳风压力的磁断反应与地球相似.
- 控制磁断层动态的物理原理在不同的行星上都保持不变.
- 在木星的磁断层中存在一个独特的边界层.
相关概念视频
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A moving charge or a current creates a magnetic field in the surrounding space, in addition to its electric field. The magnetic field exerts a force on any other moving charge or current that is present in the field. Like an electric field, the magnetic field is also a vector field. At any position, the direction of the magnetic field is defined as the direction in which the north pole of a compass needle points.
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Magnetic Field Lines
The representation of magnetic fields by magnetic field lines is very useful in visualizing the strength and direction of the magnetic field. Each of the magnetic field lines forms a closed loop. The field lines emerge from the north pole (N), loop around to the south pole (S), and continue through the bar magnet back to the north pole.
Magnetic field lines follow several hard-and-fast rules:
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Diamagnetism
Materials consisting of paired electrons have zero net magnetic moments. However, when these materials are placed under an external magnetic field, the moments opposite to the field are induced. Such materials are called diamagnets. Diamagnetism is the response of the diamagnets when placed in an external magnetic field.
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