日本地球惑星科学連合2016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-EM03] Mesosphere-Thermosphere-Ionosphere Coupling in the Earth's Atmosphere

2016年5月22日(日) 09:00 〜 10:30 A01 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*Liu Huixin(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)、齊藤 昭則(京都大学大学院理学研究科地球物理学教室)、Chang Loren(Institute of Space Science, National Central University)、新堀 淳樹(京都大学生存圏研究所)、座長:新堀 淳樹(京都大学生存圏研究所)

10:15 〜 10:30

[PEM03-05] 3-years Occurrence Variability of Concentric Gravity Waves in the Mesopause Observed by IMAP/VISI

*Septi Perwitasari1Takeshi Sakanoi1Takuji Nakamura2Mitsumu K. Ejiri2Masaki Tsutsumi2Yoshihiro Tomikawa2Yuichi Otsuka3Atsushi Yamazaki4Akinori Saito5 (1.Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University、2.National Institute of Polar Research、3.Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Japan、4.JAXA/ISAS、5.Geophysics Department, Kyoto University, Kyoto, Japan)

キーワード:Concentric gravity wave, O2 nightglow emission, Mesopause

We report the first statistical study on concentric gravity waves (CGWs) in the mesopause by using 3 years data obtained by IMAP/VISI. 235 CGWs events were found with horizontal wavelength ranging from 40 to 250 km and maximum radius of 200 to 3000 km. Occurrence of the CGWs was significantly higher during non-solstice months (February-May and August–November) than solstice months (June-July and December-January), suggesting low to moderate wind are preferable for CGWs upward propagation. The latitudinal distribution of the CGWs centers had peaks in mid latitude (40°N and 40°S) and minimum at low latitude (10°S). More events were found in the summer hemisphere mid-latitudes, with a clear transition between north and south hemisphere around equinoxes. The information of the preferable regions seen in the global distribution map and the seasonal distribution could be useful for region and seasonal selection of CGWs’ future studies.