日本地球惑星科学連合2018年大会

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[EE] Eveningポスター発表

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-EM13] 太陽地球系結合過程の研究基盤形成

2018年5月20日(日) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 7ホール)

コンビーナ:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所、共同)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)

[PEM13-P07] A survey of conditions for artificial aurora experiments at EISCAT Tromsø site using dynasonde data

*津田 卓雄1Rietveld Michael2Kosch Michael3大山 伸一郎4細川 敬祐1野澤 悟徳4川端 哲也4水野 亮4小川 泰信5 (1.電気通信大学、2.EISCAT Scientific Association、3.South African National Space Agency、4.名古屋大学、5.国立極地研究所)

キーワード:人工オーロラ、電離圏加熱、EISCAT、トロムソ、ダイナゾンデ

We report a brief survey of conditions for artificial aurora optical experiments in F region heating with O-mode at EISCAT Tromsø site using dynasonde data from 2000 to 2017. According to the results from our survey, we can find the following: the possible condition for the artificial aurora experiments is concentrated on twilight hours in both evening and morning, compared with late night hours; the possible condition appear in fall, winter, and spring while there is no chance in summer, and the month-to-month variation among fall, winter, and spring is not so clear. The year-to-year variation is well correlated with the solar cycle, and experiments during the solar minimum would be almost hopeless. These findings are useful for planning future artificial aurora optical experiments.