日本地球惑星科学連合2014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-EM09_29PM2] VarSITI - Variability of the Sun and Its Terrestrial Impact

2014年4月29日(火) 16:15 〜 16:45 501 (5F)

コンビーナ:*塩川 和夫(名古屋大学太陽地球環境研究所)、坂尾 太郎(独立行政法人宇宙航空研究開発機構 宇宙科学研究所 太陽系科学研究系)、廣岡 俊彦(九州大学大学院理学研究院地球惑星科学部門)、座長:鈴木 臣(名古屋大学太陽地球環境研究所)、江尻 省(国立極地研究所)

16:30 〜 16:45

[PEM09-44] Contribution of the Optical Mesosphere Thermosphere Imagers (OMTIs) to VarSITI

*大塚 雄一1塩川 和夫1 (1.Solar-Terrestrial Environment Laboratory, Nagoya University)

キーワード:airglow, ionosphere, thermosphere, mesosphere, gravity wave, traveling ionospheric disturbance

The Optical Mesosphere Thermosphere Imagers (OMTIs) consist of thirteen all-sky cooled-CCD imagers, five Fabry-Perot interferometers (FPIs), three meridian scanning photometers, and four airglow temperature photometers. They measure two-dimensional pattern, Doppler wind, and temperature through airglow emissions from oxygen (wavelength: 557.7 nm) and OH (near infrared band) in the mesopause region (80-100 km) and from oxygen (630.0 nm) in the thermosphere/ionosphere (200-300 km). They are in automatic operation at Australia, Indonesia, Thailand, far-east Russia, Japan, Canada, Hawaii, and Norway. Station information and quick look plots are available at http://stdb2.stelab.nagoya-u.ac.jp/omti/. We show recent results obtained by OMTIs particularly focusing on the penetration of short-period gravity wave from the lower atmosphere to the thermosphere and the ionosphere, which are often recognized as meridum-scale traveling ionospheric disturbances (MSTIDs) in the ionosphere. We also show some results obtained by the multi-point Fabry-Perot interferometers. These observations will contribute the next SCOSTEP program VarSITI, particularly to the ROSMIC Project.