日本地球惑星科学連合2019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-EM10] Multi-scale Coupling in the Magnetosphere-Ionosphere-Thermosphere System

2019年5月27日(月) 15:30 〜 17:00 A05 (東京ベイ幕張ホール)

コンビーナ:Yue Deng(University of Texas at Arlington)、Toshi Nishimura(Boston University)、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)、Yanshi Huang(Harbin Institute of Technology, Shenzhen)、座長:Yue Deng(University of Texas at Arlington)、Huixin Liu(Kyushu University, Japan)、Yanshi Huang(Harbin Institute of Technology, Shenzhen, China)、Yukitoshi Nishimura(Boston University)

16:45 〜 17:00

[PEM10-06] Meso-scale forcing in the upper atmosphere: sources and impacts

*Yue Deng1Qingyu Zhu1Cissi Lin1 (1.University of Texas at Arlington)

キーワード:Meso-scale forcing , upper atmosphere, Joule heating, Gravity waves

We present a systematical study crossing both data analysis and model simulation to improve the specification of the energy and momentum inputs into the ionosphere-thermosphere (IT) system, especially at the meso-scale, and the system response. Our results are organized in two parts. First, two-years of Swarm satellite field-aligned current (FAC) data have been analyzed in order to study the distributions of mean pattern and variability of FACs on different scales (small scale: <150 km; mesoscale: 100~500 km; large scale: >500 km). The FAC distributions are then implemented in the Global Ionosphere-Thermosphere Model (GITM) to assess relative contributions of FACs at different scales to Joule heating. To enhance our capability to directly simulate the meso- and small-scale structures, GITM has been improved with a local patch grid refinement capability. Utilizing GITM with the new grid structure, the meso- and small-scale gravity wave perturbations have been included at the lower boundary of GITM to simulate the influence of meso- and small-scale gravity waves on the upper atmosphere.