日本地球惑星科学連合2015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-EM27] 大気圏・電離圏

2015年5月26日(火) 11:00 〜 12:45 A01 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*大塚 雄一(名古屋大学太陽地球環境研究所)、津川 卓也(情報通信研究機構)、川村 誠治(独立行政法人 情報通信研究機構)、座長:冨川 喜弘(国立極地研究所)、柿並 義宏(高知工科大学システム工学群)

11:15 〜 11:30

[PEM27-12] Chemical Releaseを用いたカスプ領域大気風・プラズマドリフト同時計測 ~初期結果~

*柿並 義宏1木原 大城1渡部 重十2山本 真行1Mark Conde3Miguel Larsen4 (1.高知工科大学、2.北海道情報大学、3.アラスカ大学フェアバンクス校、4.クレムソン大学)

キーワード:カスプ, 中性大気風, プラズマドリフト, 宇宙花火, ガス放出ロケット実験, 中性大気密度異常

A chemical release experiment was taken place on 24 November 2014 to measure neutral wind and plasma drift in the cusp region, which was named the Cusp Region Experiment (C-REX). We set up 2 cameras (one for neutral Barium (Ba) and the other for ionized Barium (Ba+)) at Longyerben and Ny-Alsund for each site. In addition, one video camera at Ny-Alsund and one camera with a grating at Longyerben were set up. The rocket was launched from Andoya at 08:05 UT and first chemical release was observed at 08:14:19 UT from Longyerben, Ny-Alsund and an airplane. Ten of 24 canisters were successfully ignited between 200 and 400 km altitude at about 600 km away from Svalbard islands. Each canister contains barium (Ba) and strontium (Sr). Evaporated gasses reflect sunshine and green and blue “space fireworks” were observed by digital cameras with filter and video as well as human eyes. The filters were developed to observe resonance scattering of neutral Ba (552.5 nm) and ionized Ba (454.5 nm), and evaluated with an integrating sphere in National Institute of Polar Research. We also observed space fireworks with a grating and successfully obtained spectrums. In this paper, we introduce our observation and show preliminary results of the experiment.