苏梅克-列维9号彗星与木星磁层的电动力学相互作用

O. Bolin, N. Brenning
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引用次数: 0

摘要

预计将于1994年7月20日左右撞击木星的苏梅克-列维9号彗星与木星之间的电动力学相互作用已被研究。这颗彗星由一列由中性气体云包围的大约21个原子核组成。由于电子冲击电离和光电离,中性云在穿过磁层中的等离子体时会被部分电离。彗星向木星的运动和木星磁层在20r {sub J}内的共同旋转都有助于使云中的等离子体以穿过B的速度,因此在彗星的静止框架中产生了感应电场。作者在这里讨论了木星和电离彗星云之间的电动力学相互作用可能驱动的过程,可以在舒梅克-列维9号撞击木星本身之前观察到。幸运的是,在木星的磁层中已经有一个合适的物体可以作为这种相互作用的模型的基础:木星-木卫一系统已经被描述为一个大导体和相对运动的磁化等离子体之间耦合的原型。在木星-木卫一系统中,几毫安的电流沿着磁场长距离流动。与这些电流相关的是木星十度辐射,这是太阳系中最强的射电源之一,其激发机制仍未完全了解。舒梅克-列维彗星理论上可以以不低于木卫一的速度向木星磁层提供离子,并且相对于木星有更高的速度,因此可以想象,它可以驱动类似的过程。基于一个数值模型,作者预测任何由苏梅克-列维9号彗星与木星磁层相互作用引起的电磁辐射都将是相当微不足道的,而且很难探测到。«少
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Electrodynamical Interaction Between Comet Shoemaker-levy 9 And Jupiter's Magnetosphere
The electrodynamical interaction between Jupiter and comet Shoemaker-Levy 9, which is expected to impact on Jupiter around July 20, 1994, has been investigated. The comet consists of a train of 21 or so nuclei surrounded by neutral gas clouds. Because of electron impact ionization and photo-ionization the neutral clouds will become partly ionized when they pass through the plasma in the magnetosphere. Both the comet`s motion towards Jupiter and the co-rotation of the Jovian magnetosphere inside 20 R{sub J} contribute to give the plasma in the clouds a velocity across B, and thus an induced electric field is produced in the comet`s rest frame. The authors discuss here the possibility that the electrodynamical interaction between Jupiter and the ionized comet clouds might drive processes which can be observed prior to the impact of Shoemaker-Levy 9 on Jupiter itself. Fortunately there is already a suitable object within the Jovian magnetosphere on which to base a model for such interaction: the Jupiter-Io system has been described as an archetype for the coupling between a large conductor and a magnetized plasma in relative motion. In the Jupiter-Io system, currents of several MA flow long distances along the magnetic field. Associated with these currentsmore » is the Jovian Decametric Radiation, one of the strongest radio sources in the solar system, and for which the excitation mechanisms is still not completely understood. The Shoemaker-Levy comet can theoretically supply ions to Jupiter`s magnetosphere at a rate not so far below Io`s, and will have a higher velocity relative to Jupiter, and could therefore conceivably drive similar processes. Based on a numerical model, the authors predict that any electromagnetic radiation caused by the interaction between comet Shoemaker-Levy 9 and the Jovian magnetosphere will be rather insignificant and very difficult to detect.« less
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