日本地球惑星科学連合2022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-AS06] 台風研究の新展開~過去・現在・未来

2022年5月22日(日) 10:45 〜 12:15 201A (幕張メッセ国際会議場)

コンビーナ:辻野 智紀(気象研究所)、コンビーナ:金田 幸恵(名古屋大学宇宙地球環境研究所)、伊藤 耕介(琉球大学)、コンビーナ:宮本 佳明(慶應義塾大学 環境情報学部)、座長:辻野 智紀(気象研究所)、金田 幸恵(名古屋大学宇宙地球環境研究所)


10:45 〜 11:00

[AAS06-01] The warm-core structure of typhoons as observed through the T-PARCII aircraft reconnaissance and upper-air soundings

★Invited Papers

*Hiroyuki Yamada1,2Kosuke Ito1,2Soichiro Hirano1Kazuhisa Tsuboki3,2Taro Shinoda3、Masaya Kato3Sachie Kanada3Tadayasu Ohigashi4Satoki Tsujino5Udai Shimada5,2、Tetsuo Nakazawa5Norio Nagahama6、Kensaku Shimizu6Takeshi Horinouchi7,2Nobuhiro Takahashi3Shingo Shimizu4、 Masashi Minamide8 (1.University of the Ryukyus、2.Typhoon Science and Technology Research Center, Yokohama National University、3.Nagoya University、4.National Research Institute for Earth Science and Disaster Resilience、5.Meteorological Research Institute, Japan Meteorological Agency、6.Meisei Electric Co. Ltd.、7.Hokkaido University、8.University of Tokyo)

キーワード:Tropical cyclone intensity, Warm-core structure, Aircraft reconnaissance

Upper-tropospheric reconnaissance flights were carried out for three intense typhoons (Lan in 2017, Trami in 2018, and Mindulle in 2021) using a civil jet with a dropsonde system. In all flights, we succeeded to fly into the eye and to deploy dropsondes near the circulation center. In addition, the eye of two tropical cyclones (Ampil and Trami in 2018) were observed using radiosondes launched from stations in the Ryukyu islands. These in-situ observations provide opportunities to examine the vertical structure of the warm core in a very fine resolution (10~15 meters) between the Earth surface and the upper troposphere (~13 km MSL). They also provide opportunities to clarify a relationship between the warmth of the circulation center and the typhoon intensity in a direct way, which will be helpful for improving intensity estimation using a satellite-based microwave temperature sounder. In this work, we examined the warm-core structure of these typhoons and the relationship between the warm core and the typhoon intensity. In each sounding, the temperature anomaly of the warm core was defined as the difference in temperatures between the eye and the surrounding region (radius of 550-600 km). The mean temperature anomaly between 900 and 250 hPa was plotted as a function of the sea-level pressure (as shown figure). There is a robust strong positive relationship between strength of the warm core and typhoon intensity, as should be expected for a balanced vortex. However, comparing some observations of Mindulle (plotted as M) and Lan (L), the temperature anomalies are almost the same (8-10 K) even though the sea-level pressures differ by about 10 hPa. This suggests not only hydrostatic equilibrium, but also other factors involved in the determination of the minimum sea-level pressure of a typhoon.