日本地球惑星科学連合2021年大会

講演情報

[J] ポスター発表

セッション記号 M (領域外・複数領域) » M-SD 宇宙開発・地球観測

[M-SD40] 将来の衛星地球観測

2021年6月4日(金) 17:15 〜 18:30 Ch.20

コンビーナ:本多 嘉明(千葉大学環境リモートセンシング研究センター)、高薮 縁(東京大学 大気海洋研究所)、Shinichi Sobue(Japan Aerospace Exploration Agency)、山本 晃輔(国立研究開発法人宇宙航空研究開発機構)

17:15 〜 18:30

[MSD40-P11] 全球風観測プログラム(2)

*木村 俊義1、岡本 創2、境澤 大亮1、橋本 真喜子1 (1.宇宙航空研究開発機構、2.九州大学)

キーワード:風、衛星観測、全球観測

Observation of wind is the last part in Satellite Earth Observation. The difficulties of the wind observation are its 3-D structure and precision of measurement. Recent weather satellite observation made it possible using AMV technique with a few channels. Using future infrared sounder on the next generation weather satellite, more fine vertical structure with global coverage data than of current satellite, will be observed. However vertical structure and wind vector determination are only possible through numerical model. To keep the precision of such data, wind Lidar satellites are expected. The first wind Lidar satellite ADM-Aelous was launched already and getting more precise data than using infrared sounder. But the observation capability of Lidar limits its observation area. To get global 3-D wind measurement data, we are studying about the combination of these two sensors. This year we will report temporal expected performances of new infrared sounder and wind lidar.