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首页> 外文期刊>Geophysical Research Letters >Effect plasmaspheric drainage plumes on solar-wind/magnetosphere coupling
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Effect plasmaspheric drainage plumes on solar-wind/magnetosphere coupling

机译:等离子层羽流对太阳风/磁层耦合的影响

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摘要

[ 1] Evidence is uncovered that plasmaspheric drainage plumes flowing into the dayside reconnection site mass load the reconnection rate and thereby reduce the coupling of the solar wind to the Earth's magnetosphere. Solar-wind/magnetosphere coupling is statistically analyzed with the 1963-2003 OMNI2 data set matched up with the AE, AU, and PCI geomagnetic indices. Times when plasmaspheric drainage plumes are flowing are discerned using multiple spacecraft with plasma detectors in geosynchronous orbit. It is found that for a given value of -vB(z) of the solar wind, the geomagnetic indices AE, AU, and PCI are statistically lower when plasmaspheric drainage plumes are present than when plumes are not present. This is taken as a measure of a weakened coupling of the solar wind to the Earth's magnetosphere caused by the plumes. An Addendum examines the effects of polar-cap saturation on the auroral electrojet index.
机译:[1]有证据表明,流向白天重新连接站点的等离子层排水羽会给重新连接率带来负担,从而减少了太阳风与地球磁层的耦合。利用1963年至2003年的OMNI2数据集对AE,AU和PCI地磁指数进行匹配,对太阳风/磁层耦合进行了统计分析。使用多台航天器和地球同步轨道上的等离子探测器,可以确定等离子层流羽流动的时间。发现对于给定的太阳风的-vB(z)值,当存在​​等离子层排水羽流时,地磁指数AE,AU和PCI在统计上要比不存在羽流时低。这是由于羽流导致太阳风与地球磁层减弱耦合的一种措施。附录检查了极帽饱和度对极光电喷射指数的影响。

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