High-Speed Imaging of Sprite Streamers

被引：3

作者：

McHarg, Matthew G. ^{[1
]}

Stenbaek-Nielsen, Hans C. ^{[2
]}

Kanmae, Takeshi ^{[2
]}

Haaland, Ryan K. ^{[3
]}

机构：

[1] USAF Acad, Dept Phys, Colorado Springs, CO 80840 USA

[2] Univ Alaska, Inst Geophys, Fairbanks, AK 99775 USA

[3] Ft Lewis Coll, Dept Phys & Engn, Durango, CO 81301 USA

来源：

IEEE TRANSACTIONS ON PLASMA SCIENCE | 2011年 / 39卷 / 11期

基金：

美国国家科学基金会;

关键词：

Plasma applications; plasma diagnostics; plasma stability; VIDEO;

D O I：

10.1109/TPS.2011.2165299

中图分类号：

O35 [流体力学]; O53 [等离子体物理学];

学科分类号：

070204 ; 080103 ; 080704 ;

摘要：

The spatial and temporal developments of sprite streamers in the mesosphere are discussed in the context of the data recorded on August 27, 2009. Streamers initiate at approximately 75 km in altitude and are seen to propagate first downward and subsequently upward. Streamer splitting is observed as the streamers propagate. The streamer tips are approximately three times brighter than the planet Jupiter.

引用

页码：2266 / 2267

页数：2

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