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Measurement of Auroral Electric Fields with an Antarctic Sounding Rocket S-310JA-7. 2.AC Electric Field

机译:用南极探空火箭s-310Ja-7测量极光电场。 2.aC电场

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摘要

A sounding rocket with double-probes for DC electric field and AC electric field (5-220Hz band) measurement was launched from Syowa Station in Antarctica around the onset time of an intense auroral substorm. The rocket first encountered a poleward expanding auroral arc, where intense (1.4mV/m) and broad band electric field fluctuations were measured around the arc at the altitude of 105-128km. The rocket then moved across an equatorward drifting arc, where narrow-band electric field fluctuations around 40Hz were measured at the altitude of ∿190km. Considering the DC electric field data and the electron density gradient observed on the same rocket, it is likely that the former fluctuation is due to drift waves or ion acoustic waves excited by the cross-field type or two-stream type plasma instability, while the latter is due to electrostatic ion cyclotron waves excited by fieldaligned currents.
机译:在强烈的极光亚暴的爆发时间附近,从南极洲的Syowa站发射了用于测量直流电场和交流电场(5-220Hz频带)的双探头探空火箭。火箭首先遇到极向扩展的极光弧,在105-128km的高度上,在弧周围测得了强烈的(1.4mV / m)和宽带电场起伏。然后,火箭越过赤道漂移弧,在190km的高度上测量了40Hz附近的窄带电场起伏。考虑到在同一枚火箭上观察到的直流电场数据和电子密度梯度,前者的波动很可能是由于交叉场型或两流型等离子体不稳定性激发的漂移波或离子声波而引起的,而后者归因于场定向电流激发的静电离子回旋波。

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