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-EM10] Study of coupling processes in solar-terrestrial system

2015年5月28日(木) 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:*山本 衛(京都大学生存圏研究所)、野澤 悟徳(名古屋大学太陽地球環境研究所)、小川 泰信(国立極地研究所)、橋口 浩之(京都大学生存圏研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)、座長:吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)

12:00 〜 12:15

[PEM10-15] Ground-based network observations of wind and temperature of the thermosphere using five Fabry-Perot interferometers

*塩川 和夫1中村 義弘1大山 伸一郎1大塚 雄一1 (1.名古屋大学太陽地球環境研究所)

キーワード:地上多点観測, 地上観測ネットワーク, ファブリ・ペロー干渉計, 熱圏, 電離圏, 超高層大気

It is well known that dynamic variation of Earth's ionosphere affects human activities in space through interference on the ground-satellite radio communications and degradation of GNSS positioning accuracy. The measurement of wind and temperature of the thermosphere is essentially important to understand dynamic variation of the ionosphere, because collision with neutral atmosphere is a dominant force to cause ionospheric plasma variation. High-resolution interferometry of airglow emissions using Fabry-Perot or Michelson interferometers is the unique technique to make remote sensing of the thermospheric wind and temperature from the ground. Since 2011, the Solar-Terrestrial Environment Laboratory (STEL), Nagoya University have been operating five Fabry-Perot interferometers (FPIs) at Shigaraki (Japan, FP00), Tromsoe (Norway, FP01), Chiang Mai (Thailand, FP02), Kototabang (Indonesia, FP03), and Darwin (Australia, FP04). They measure thermospheric wind and temperature through Doppler shift of the 630-nm airglow emission that has an emission layer at altitudes of 200-300 km. The use of 70mm-diameter etalons for FP02-FP04 makes the cost of the FPIs about three times lower than those with 116mm-diameter etalons for FP00 and FP01. By revising procedure of fringe-center determination we obtained reliable temperature of the thermosphere with accuracies of 10-40 K using these small-etalon FPIs. In this presentation, we show recent results of thermospheric and ionospheric dynamics obtained by these five FPIs.