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22日(月) 09:00 〜 10:15 101 (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)、Chairperson:Yue Deng(University of Texas at Arlington)、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)


09:45 〜 10:00

[PEM12-24] Improvements of multi-scale geomagnetic forcing specification from the ground-based integrated networks and the impacts on I-T modeling

*Yue Deng1、Cheng Sheng1、Toshi Nishimura2、William Bristow3、Christine Gabrielse4、Shunrong Zhang5、Larry Lyons6 (1.University of Texas at Arlington、2.Boston University、3.Pennsylvania State University、4.Aerospace Corporation、5.MIT Haystack Observatory、6.University of California Los Angeles)

キーワード:Ionosphere-thermosphere modeling, multi-scale forcing, ground-based observations

Techniques developed in the past few years enable the derivation of high-resolution regional ion convection and particle precipitation patterns from the Super Dual Auroral Radar Network (SuperDARN) and All-Sky Imager (ASI) observations, respectively. In this study, global ionosphere-thermosphere model (GITM) is driven by the high-resolution patterns derived from those new observational capabilities to simulate the I-T response during the March 26, 2014 event. It is found that multi-scale ion convection forcing estimated from high-resolution SuperDARN observations has a very strong meso-scale component, which increases the regional Joule heating by 30% on average. The meso-scale electron precipitation derived from ASI measurements contributes to 30% of the total electron energy flux, and its impact on the neutral density and winds is comparable to the meso-scale convection forcing estimated from SuperDARN observations. Both meso-scale convection and precipitation forcing are found to strongly enhance ionospheric and thermospheric disturbances, especially at meso-scale.