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- SA13D-1942: Statistical Distribution of Dawnside Auroral Polarization Streams
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Board 1942‚ Hall EFG (Poster Hall)NOLA CC
Author(s):Generic 'disconnected' Message
Jiang Liu, University of California Los Angeles (First Author, Presenting Author)
Colin Forsyth, UCL Mullard Space Science Laboratory
Larry Lyons, University of California Los Angeles
Chih-Ping Wang, University of California Los Angeles
Vassilis Angelopoulos, University of California Los Angeles
Andrei Runov, University of California Los Angeles
Sheng Tian, University of California Los Angeles
Yangyang Shen, University of California Los Angeles
Johnathan Burchill, University of Calgary
Milan Stephen, University of Leicester
The dawnside auroral polarization stream is a unique type of plasma wind in Earth′s high-latitude ionosphere. These streams play a key role in shaping the aurora and affecting how energy enters from space into the atmosphere. In this study, we explore when and where these streams are most likely to occur. The results not only help us better understand what causes them but also increase the ability to predict space weather events related to them, such as variations in atmosphere temperature.
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