日本地球惑星科学連合2016年大会

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口頭発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS14] 大気電気学

2016年5月23日(月) 15:30 〜 17:00 203 (2F)

コンビーナ:*三浦 和彦(東京理科大学理学部)、鴨川 仁(東京学芸大学教育学部物理学科)、座長:森本 健志(近畿大学理工学部)

16:15 〜 16:30

[MIS14-10] 偏波フェーズドアレイレーダの開発とビーム形成に関する検討

*菊池 博史1呉 亭1金 寛1牛尾 知雄1後藤 秀人2水谷 文彦2 (1.大阪大学大学院工学研究科、2.東芝)

キーワード:気象レーダ、フェーズドアレイアンテナ

Development of a polarimetric phased array weather radar as a subsequent project of the phased array weather radar (PAR) is under discussion. The design of a polarimetric phased array weather radar has been the object of several experimental development. The polarimetric phased array weather radar has significantly advanced the following points. 1) to classify types of precipitation, 2) to provide quantitative estimates of precipitation accumulation, 3) to obtain high spatial and temporal resolution volumetric radar data. 1) and 2) are contributed by a polarimetric sensing technique, and 3) is provided by the digital beam forming techniques in a phased array radar system. In this paper, precipitation radar signal simulations based on the under considering radar concept are carried out to discuss the estimation accuracy of polarimetric precipitation profiles (differential reflectivity, specific differential phase, and copolar correlation coefficient) with two DBF methods that are based on Fourier and minimum mean square error (MMSE) methods. The comparison of the performance of the two methods indicates that MMSE is superior in an observation accuracy because of the effect of a stable and robust main lobe and adaptively suppressed side lobes.