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首页> 外文期刊>Geophysical Research Letters >Jupiter's magnetospheric change by Io's volcanoes
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Jupiter's magnetospheric change by Io's volcanoes

机译:木卫一的火山对木星的磁层变化

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摘要

Monitoring observations of Jupiter's sodium nebula and [SII] 673.1 nm emission from the Io plasma torus were made for 20 days in 2003. During these observations, the brightness of the sodium nebula showed a small enhancement which seemed to be caused by Io's volcanic outburst. During this enhancement, [SII] 673.1 nm brightness and the ion temperature (scale height) along Jupiter's magnetic fields did not show any significant change, but magnetic flux tube content of S~+ ion was calculated from the [SII] 673.1 nm brightness and the scale height, and an increase of the ion flux tube content was clearly identified. Thus, increase of supplied plasma from Io seems to be reflected in both plasma density and ion temperature. We conclude that Io's volcanic enhancement with a duration time of a few days can change Jupiter's inner magnetospheric environment in aspects of both ion density and temperature.
机译:2003年对木星钠星云和来自Io等离子体圆环的[SII] 673.1 nm发射进行了监测观察,观测了20天。在这些观察中,钠星云的亮度显示出小幅增强,这似乎是由Io的火山爆发引起的。在此增强过程中,[SII] 673.1 nm亮度和沿木星磁场的离子温度(标度高度)没有显示任何显着变化,但是根据[SII] 673.1 nm亮度和可以清楚地看到水垢高度和离子通量管含量的增加。因此,从Io提供的等离子体的增加似乎反映在等离子体密度和离子温度上。我们得出的结论是,持续时间为几天的Io火山增强可以在离子密度和温度方面改变木星内部的磁层环境。

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