日本地球惑星科学連合2019年大会

講演情報

[J] 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-IS27] 大気電気学:大気電気学研究の自然災害軽減への応用

2019年5月28日(火) 09:00 〜 10:30 202 (2F)

コンビーナ:芳原 容英(電気通信大学 大学院情報理工学研究科)、鴨川 仁(東京学芸大学教育学部物理学科)、座長:森本 健志

09:00 〜 09:15

[MIS27-01] Advantage and Disadvantage of the Phased Array Weather Radar

*牛尾 知雄1妻鹿 友昭1菊池 博史2吉川 栄一3 (1.首都大学東京、2.電気通信大学、3.宇宙航空研究開発機構)

Recent progress of information and communication technologies has been enabling us to realize a rapid scanning radar system. In 2012, Toshiba Corporation and Osaka University succeeded in developing a new type of Phased Array Radar (PAR) system (Yoshikawa et al. 2013, Ushio et al. 2015, Mizutani et al. 2018) under a grant of National Institute of Communication and Information Technology (NICT), and installed in Suita Campus, Osaka University. This PAR system can scan the whole sky within 30 seconds up to 60 km in radius over 100 elevation angles with digital beam forming technique, and the initial observation results demonstrate the unique capability of the new PAR system. However, the observation is sometimes seriously contaminated by strong ground clutter through relatively high sidelobes at transmitting stage. In this study, a new clutter mitigation algorithm from adaptive beam forming technique on Minimum Mean Square Error (MMSE) formulation was investigated, and succeeded in suppressing not only the ground clutter but also ghost echo from strong precipitation echo nearby more than 20dB. And also the adaptive algorithm was applied to supress the range sidelobe and showed the sidelobe level of -60dB. In this presentation, the advantages and disadvantages of the PAR will be discussed based on the observation results.