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Measurement of Auroral Electric Fields with an Antarctic Sounding Rocket S-310JA-7. 1.DC Electric Field

机译:用南极探空火箭s-310Ja-7测量极光电场。 1.DC电场

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摘要

The results are given on the DC electric field in an active auroral arc and outside the equatorside of it observed with two pairs of orthogonal double probes launched by an Antarctic sounding rocket S-310JA-7 at 191550 UT on March 27,1978 at Syowa Station. The north-south component of the observed electric field was northward (equatorward) in the arc, and southward (poleward) outside the equatorside of the arc with a magnitude of about 20mV/m. The east-west component was mostly westward throughout the rocket flight and smaller (about 5mV/m) in the arc and larger (about 50mV/m) outside the arc. Anticorrelation of the electric field and precipitating particles is evident. An examination of the oppositely inward directed electric fields in the meridional cross section suggests an electrostatic potential configuration responsible for the acceleration of precipitating particles. The observed westward component would have been originated in the large scale earthward plasma convection in the magnetosphere.
机译:结果是在活跃的极光弧和赤道外的直流电场上给出的,1978年3月27日,南极探空火箭S-310JA-7在191550 UT在Syowa站观测了两对正交双探针。 。所观察到的电场的南北分量在弧的北(赤道)方向,在弧的赤道侧向南(极)方向,幅度约为20mV / m。在整个火箭飞行过程中,东西向的分量大部分是向西的,弧段较小(约5mV / m),弧段较大(约50mV / m)。电场和沉淀颗粒的反相关是显而易见的。对子午线横截面中向内相反方向的电场的检查表明,静电势能结构负责沉淀颗粒的加速。观测到的向西分量可能起源于磁层中大规模的向地等离子对流。

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