日本地球惑星科学連合2023年大会

講演情報

[E] 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-EM12] Coupling Processes in the Atmosphere-Ionosphere System

2023年5月21日(日) 10:45 〜 12:00 101 (幕張メッセ国際会議場)

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)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Chang Loren(Institute of Space Science, National Central University)、Yue Deng(University of Texas at Arlington)、座長:Lin Charles(Department of Earth Sciences, National Cheng Kung University)、斎藤 享(国立研究開発法人海上・港湾・航空技術研究所電子航法研究所)


11:00 〜 11:15

[PEM12-07] Atmospheric and Ionospheric Responses to Hunga-Tonga Volcano Eruption Simulated by WACCM-X

★Invited Papers

*Hanli Liu1、Wenbin Wang1、Joseph D Huba2、Peter H Lauritzen3、Francis Vitt1,4 (1.National Center for Atmospheric Research, High Altitude Observatory、2.Syntek Technologies、3.National Center for Atmospheric Research, Climate and Global Dynamics、4.National Center for Atmospheric Research, Atmospheric Chemistry Observations and Modeling)

キーワード:whole atmosphere modeling, Lamb wave, volcano eruption

Numerous observations have shown large global responses to the Hunga Tonga-Hunga Ha'apai Volcano Eruption on January 15 2022 in the lower, middle and upper atmosphere. It is of interest to simulate this event using a whole atmosphere model, in order to better understand the physical processes involved, interpret the observations, and also to test the model capability. In this study, the NCAR Whole Atmosphere Community Climate Model with thermosphere/ionosphere extension (WACCM-X) is used to simulate this event. High spatial resolution configuration is used, with horizontal resolution of ~25km and vertical resolution of 0.1 scale height in most of the middle and upper atmosphere. The model is initialized with a surface pressure perturbation around the epicenter. The magitude of the initial perturbation is choosen to produce propagating surface pressure perturbations consistent with observations. The model simulates Lamb waves with increasing wind and temperature amplitudes with altitude, reaching over 100m/s and 100K, respectively, in the thermosphere. Large perturbations in ionospheric ExB drifts and strong traveling ionospheric disturbations (TIDs) are also simulated, with magitudes comparable with observations. Detailed analysis of the wave structures will be presented in this talk.