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-EM06] Mesosphere-Thermosphere-Ionosphere Coupling in the Earth's Atmosphere

2015年5月27日(水) 14:15 〜 16:00 A01 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*Huixin Liu(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、大塚 雄一(名古屋大学太陽地球環境研究所)、Libo Liu(Institute of Geology and Geophysics, Chinese Academy of Sciences)、新堀 淳樹(京都大学生存圏研究所)、座長:Larisa Goncharenko(Massachusetts Institute of Technology Haystack Observatory)

15:15 〜 15:30

[PEM06-21] All-sky measurements of short period waves nightglow emissions

*Igor KOLTOVSKOI1Petr AMMOSOV1Galina GAVRILYEVA1Anastasia AMMOSOVA1 (1.Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy)

キーワード:internal gravity waves, mesosphere, hydroxyl

Will present the results of statistical analysis of the parameters of internal gravity waves registered on the variations of emission hydroxyl molecule. Wave patterns registered infrared all-sky camera installed on the optical station Maimaga (Yakutia). Analyzed data received during the winter period 2008-2013. 118 waves were registered, most of which propagated in a westerly direction. For the wave length range from 15 - 70 km (average value is - 29km) observed horizontal phase velocity varies from 17 to 140.8 m / s (average is -57m / s) and the estimated periods are within 7-40 min (the average is - 9min). Statistical characteristics of the waves do not differ from the results of the registration of such waves at middle and low latitudes. The azimuthal distribution of the direction of wave propagation is consistent with the theory of filtering background wind waves in the middle atmosphere. Probable sources of waves are assumed to mountain ranges, located 200 km to the east of the place of observation. There are a few large values of the average wavelength and wave propagation velocity than those registered at lower latitudes. Apparently, this is due to lower energy loss and wave velocity in passing from the source to the mesosphere, although not excluded for other reasons.
It is planned to identify all-sky measurements of short period waves in the green emission recording OI (557,7 nm) in the visible wavelength of the spectrum (the height of the airglow ~ 96 km). Will present the results of observations at two different heights (~87 and 97 km).