1993年11月15日超极弧的研究

Yongliang Zhang, D. Mcewen, K. Yumoto, K. Shiokawa, K. Hayashi
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引用次数: 1

摘要

1993年11月15日,在尤里卡(88.9°N, 318°E CGM)观测到的弧形,在雷索卢特湾(84.5°N, 316°E CGM)和剑桥湾(77.6°N, 306°E CGM)也观测到,从极冠中心延伸到夜侧椭圆形。极光活动持续了10 h,最大强度达20 kR (557.7 nm)。利用Tsyganenko的磁场模型(T89)将超极弧映射到磁尾中。发现源区位于等离子体片中央边界层,并向尾叶延伸。通过对磁特征的分析,还发现沿转极弧存在向太阳方向的电喷流。该弧发生在IMF Bz向北偏强的时期,时间由负向正变化,控制了跨极弧在黎明-黄昏方向的运动。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A Study of the November 15, 1993 Transpolar Arc
An arc observed at Eureka (88.9°N, 318°E CGM) on November 15, 1993, was also observed at Resolute Bay (84.5°N, 316°E CGM) and Cambridge Bay (77.6°N, 306°E CGM) and seen to extend from the central polar cap to the nightside oval. The auroral activity continued for 10 hours with its maximum intensity up to 20 kR (557.7 nm). The transpolar arc was mapped into the magnetotail by using Tsyganenko' s magnetic field model (T89). It is found that the source region was located at central plasma sheet boundary layer and extended to the tail lobe. It is also found that there is a sunward electrojet along the transpolar arc, based on analysis of magnetic signatures. The arc occurred during a period of strongly northward IMF Bz and time varying By, from negative to positive, which controlled the motion of the transpolar arc in the dawn-dusk direction.
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