日本地球惑星科学連合2015年大会

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インターナショナルセッション(口頭発表)

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-EM08] Progress in Physics of the Inner Magnetosphere

2015年5月26日(火) 14:15 〜 16:00 302 (3F)

コンビーナ:*Danny Summers(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)

15:40 〜 15:55

[PEM08-06] Spatial and temporal variation of Sub-Auroral Polarization Streams: Initial results from the SuperDARN HOP radars

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

キーワード:SuperDARN HOP radars, sub-auroral polarization streams, substorm

Super Dual Auroral Radar Network (SuperDARN) is a network of HF radars deployed in both hemispheres. The SuperDARN Hokkaido West radar, one of SuperDARN HOkkaido Pair of (HOP) radars, is the newest SuperDARN radar located in Rikubetsu, Hokkaido, Japan, which began its operation in October 2014. Longitudinal coverage of subauroral ionosphere over several hours of magnetic local time by the SuperDARN HOP radars, together with other midlatitude SuperDARN radars, will enable us to study the detailed characteristics of Sub-Auroral Polarization Streams (SAPS), and to find clues to their generation, growth and decay mechanisms. In this paper initial results of the SuperDARN Hokkaido Pair of (HOP) radars observation of SAPS, with focus on the location / timing of SAPS activity relative to geomagnetic activity such as substorms, will be presented.