日本地球惑星科学連合2025年大会

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[E] 口頭発表

セッション記号 A (大気水圏科学) » A-AS 大気科学・気象学・大気環境

[A-AS04] 大気の鉛直運動を基軸とした地球環境学の新展開

2025年5月30日(金) 10:45 〜 12:15 展示場特設会場 (4) (幕張メッセ国際展示場 7・8ホール)

コンビーナ:佐藤 正樹(東京大学大気海洋研究所)、佐藤 薫(東京大学 大学院理学系研究科 地球惑星科学専攻)、岡本 創(九州大学)、伊藤 純至(東北大学)、座長:佐藤 正樹(東京大学大気海洋研究所)、伊藤 純至(東北大学)

10:45 〜 11:00

[AAS04-01] Statistical Analysis and frequency Spectra of Vertical Air Velocities from MU Radar Data in the Tropopause-Stratosphere (1987-2024)

★Invited Papers

*Hubert LUCE1Noriyuki Nishi2Hiroyuki Hashiguchi1 (1.Research Institute for Sustainable Humanosphere、2.Fukuoka University)

キーワード:vertical velocity, frequency spectra, statistics, lower atmosphere

Vertical air motion is essential in various meteorological processes, but measuring it presents significant challenges. VHF Stratosphere-Troposphere radars, such as the 46.5 MHz Middle and Upper atmosphere (MU) radar at the Shigaraki MU Observatory in Japan, provide a method for measuring vertical air velocities in the tropopause-stratosphere. The MU radar has been operating since 1984, collecting routine data each month over several days. This study presents an extensive statistical analysis of vertical air velocity measurements (W ) in the altitude range of 2 to 20 km, spanning 38 years (1987–2024). We analyze mean, standard deviation, percentiles, skewness, kurtosis, and intermittency from three independent measurement methods: direct vertical measurements (W), and measurements derived from two pairs of oblique beams (WNS and WEW ), symmetrically oriented toward the North-South and East-West directions, respectively, at 10 degrees off zenith. Below 10 km, all three methods exhibit similar seasonal variations in the statistical parameters. Above 10 km, slight differences emerge, likely linked to increased static stability. Additionally, we analyze the mean slopes Sw of the frequency spectra of W within the [0.5-6 hours] period range, corresponding to the core frequency range of internal gravity waves at the MU radar latitude (36°N) (Luce et al., 2024). After accounting for previously overlooked instrumental effects, we find that: (1) in the troposphere (N2<2×10-4 rad2s-2), Sw remains nearly seasonally invariant (-0.8), despite significant variability in horizontal wind speed U , and (2) in the stratosphere (N2>2×10-4 rad2s-2), Sw varies between 0 and -1.2 and shows a clear exponential dependence on U up to 70 ms-1 . Numerical simulations show that Doppler shift effects cannot explain the U dependence. Thus, the variation of Sw with U likely reflects a real change in the intrinsic frequency spectrum's shape, which is not accounted for in current theoretical models.

Luce, H., Nishi N., Hashiguchi H. (2024) A Climatological Study of the Frequency Spectra of Vertical Winds From MU Radar Data (1987–2022), J. Geophys. Res., 129, e2024JD041677, https://doi.org/10.1029/2024JD041677