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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >The Effects of the Polar Rain on the Polar Wind Ion Outflow From the Nightside Ionosphere
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The Effects of the Polar Rain on the Polar Wind Ion Outflow From the Nightside Ionosphere

机译:The Effects of the Polar Rain on the Polar Wind Ion Outflow From the Nightside Ionosphere

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摘要

The polar wind, consisting of low-energy ions and electrons, is an outflow along the open magnetic field lines from the polar cap ionosphere to the magnetosphere. Previous studies found that both solar radiation and solar wind electromagnetic energy are the two main energy sources for the polar wind. The polar rain, being field-aligned precipitating electrons from the solar wind to the polar cap, may provide additional energies for the polar wind. This scenario is complicated as simulation studies show that polar rain changes the electric potential structures over the polar cap ionosphere. It is unclear how the polar rain affects the polar wind ion outflow. In this study, we show a positive correlation between the polar wind and the polar rain. Meanwhile, the polar wind is generally diminished in regions with strong Earth's magnetic field, suggesting the |B| modulates the penetration depth of the polar rain through the magnetic mirror force and thus the energy dissipation of the polar rain. Therefore, the polar rain can be an additional energy source for the polar wind although the polar rain has generally smaller energies and intensities than the particle precipitations in the auroral regions.
机译:极地风、低能离子和组成沿着开放磁电子,是一个流出从的极冠电离层电场线磁气圈。太阳辐射和太阳风电磁能量是两个主要的能源极地风。沉淀电子从太阳风极地冰冠,可以提供额外的能量极地风。仿真研究表明,极地雨改变了电势结构极冠电离层。极地雨影响极地风离子外流。这项研究中,我们显示正相关极地风和极地雨之间。与此同时,极地风一般消失了强劲的地区地球磁场,表明B | |调节渗透通过磁极地深雨镜像力的能量耗散,从而极地下雨。一个额外的极地风的能量来源尽管极地雨一般较小比粒子能量和强度在极光的地区降雨雪。

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