日本地球惑星科学連合2014年大会

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セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM04_28AM2] New Perspectives on Earth's Inner Magnetosphere

2014年4月28日(月) 11:00 〜 12:40 311 (3F)

コンビーナ:*Summers Danny(Dept of Math and Stats,Memorial University of Newfoundland)、海老原 祐輔(京都大学生存圏研究所)、三好 由純(名古屋大学太陽地球環境研究所)、座長:海老原 祐輔(京都大学生存圏研究所)

11:55 〜 12:10

[PEM04-04] Characteristics of dayside SAPS structures observed by the SuperDARN Hokkaido radar

*西谷 望1堀 智昭1永野 浩貴1 (1.Solar-Terrestrial Environment Laboratory, Nagoya University)

キーワード:dayside, SAPS, SuperDARN, Hokkaido radar, magnetosphere, ionosphere

Sub-Auroral Polarization Streams (SAPS) are intense westward ionospheric flows in the subauroral ionosphere, and considered to be generated as a result of magnetosphere-ionosphere coupling during relatively disturbed periods. SAPSs are usually located in the evening to midnight sector, but occasionally it extends to earlier magnetic local times close to local noon. Owing to limitation of the observation techniques, no detailed studies of its local time extent have been made so far. In this study we use the data from the SuperDARN Hokkaido radar, one of the midlatitude SuperDARN radars located at the lowest geomagnetic latitude, to discuss the detailed characteristics of dayside SAPS, with focus on their relation to solar wind and geomagnetic parameters.