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The Earth's magnetopause as a source and sink for equatorial nightside energetic charged particles

机译:地球的磁层顶是赤道夜间高能带电粒子的源和汇

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摘要

The Imaging Proton Spectrometer (IPS) and the Imaging Electron Spectrometer (IES) on the Polar satellite have measured temporary deviations in the isotropy of the pitch angle distributions (PADs) of charged particles in the inner magnetosphere. As Polar passes through the night-side equatorial region, the IPS and IES observe dropouts of charged particles with pitch angles near 90°, known as butterfly distributions caused by the shadowing of the magnetopause. Additionally, Polar observes a lower energy (<60keV) intensification of locally mirroring ions while simultaneously detecting butterfly PADs in both higher energy ions and electrons. While it is accepted that charged particles can be lost to the magnetopause due to shadowing effects, the modeling here can suggest that the magnetopause can also be a direct source for particles observed in magnetosphere, with a strong dependence upon both pitch angle and particle energy.
机译:Polar卫星上的成像质子能谱仪(IPS)和成像电子能谱仪(IES)测量了内部磁层中带电粒子的俯仰角分布(PAD)的各向同性的暂时偏差。当Polar通过夜晚的赤道区域时,IPS和IES观察到带电粒子的俯仰角接近90°时会掉落,这被称为由磁磁更年期阴影引起的蝶形分布。此外,Polar观察到局部镜像离子的能量较低(<60keV),同时检测到能量较高的离子和电子中的蝶形PAD。尽管人们公认带电粒子可能会由于遮蔽效应而流失到磁层顶,但此处的模型可以表明,磁层顶也可以是磁层中观察到的粒子的直接来源,这与俯仰角和粒子能量都有很强的依赖性。

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