用DEMETER观测白天和夜间惠斯勒等离子体顶

Chao-Yen Chen, T. Liu
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引用次数: 0

摘要

本文利用地震带电磁发射探测卫星(DEMETER)在2005-2010年白天1030lt(当地时间)和夜间2230lt(当地时间)探测到的哨声数,研究了电离层等离子体ause的位置。哨声找到了白天和夜间都能清晰分配的浆层顶位置。我们研究了不同经度、太阳活动、季节和地磁活动的夜间/日间等离子体ause。结果表明,白天等离子体顶出现在夜间等离子体顶的赤道侧。白天和夜间的等离子体层顶对太阳活动都很敏感,在研究期间,等离子体层顶由太阳活动低峰向高峰方向向赤道方向移动。等离子体顶的季节变化是相当随机和不显著的。在磁扰动条件下,等离子体顶倾向于向赤道方向移动。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Daytime and Nighttime Mapped Whistler Plasmapause Observed by DEMETER
This paper investigates the plasmapause positions in the ionosphere by measurement of the whistler count probed by DEMETER (Detection of Electro-Magnetic Emissions Transmitted from Earthquake Regions) satellite in the daytime at 1030 LT (local time) and the nighttime at 2230 LT during 2005-2010. The whistler finds the plasmapause position which can be clearly allocated in both daytime and nighttime. We examine the nighttime/daytime plasmapause in various longitudes, solar activities, seasons, and geomagnetic actives. Results show that the daytime plasmapause appears in the equatorward side of the nighttime one. Both the daytime and nighttime plasmapause are sensitive to solar activity, which move equatorward form the low to high solar activity in the study period. The seasonal variation of the plasmapause are rather random and insignificant. During magnetic disturbed condition, the plasmapause tend to move equatorward.
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