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The Diffuse Auroral Eraser

机译:分散的极光的橡皮擦

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摘要

The source of diffuse aurora has been widely studied and linked to electron cyclotron harmonic and upper-band chorus waves. It is known that these waves scatter 100s of eV to 10s of keV electrons from the plasma sheet, but the relative contribution of each wave type is still an open question. In this study, we report an interesting and unusual auroral feature observed on March 15, 2002. We believe that these observations could help further our understanding of waves associated with diffuse aurora. This diffuse auroral feature is characterized by four phases: (1) the initial phase exhibiting regular diffuse aurora; (2) the brightening phase, where an east-west auroral stripe rapidly brightens; (3) the eraser phase, where the stripe dims to below its initial state; and (4) the recovery phase, where the diffuse aurora returns to its original brightness. Using a superposed epoch analysis of 22 events, we calculate the average recovery phase time to be 20 s, although this varies widely between events. We hypothesize that the process responsible for these auroral eraser events could be the result of chorus waves modulating diffuse aurora.
机译:扩散极光被广泛的来源研究和电子回旋谐波和upper-band合唱。这些波散射100 keV的eV - 10的年代从等离子体电子板,但相对的每个波类型仍然是一个开放的贡献的问题。和不寻常的极光特性观察3月15日,2002. 帮助我们进一步的了解与分散极光。极光特性的特点是四个阶段:(1)初始阶段表现出普通扩散极光;东西方极光条纹迅速照亮;橡皮擦阶段,下面的条纹会变暗它的初始状态;扩散极光返回到原来在哪里亮度。22日事件,我们计算平均回收率阶段时间20多岁,虽然这个变化广泛的事件之间。过程中负责这些极光橡皮擦事件可以合唱波的结果调节分散极光。

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