日本地球惑星科学連合2019年大会

講演情報

[E] ポスター発表

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-EM15] 太陽地球系結合過程の研究基盤形成

2019年5月30日(木) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 8ホール)

コンビーナ:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)

[PEM15-P10] Redevelopment of the MU radar transceiver-module control system

*山本 衛1黒川 浩規1橋口 浩之1 (1.京都大学生存圏研究所)

キーワード:MUレーダー、制御システ、再開発

The MU radar was installed in Shigaraki, Japan in 1984 as the world first atmospheric radar with active phased-array antenna system. The MU radar consists of 475 Yagi antennas in the circular field of about 100m diameter. By the electronic phase shift of each Yagi, the antenna beam is steered to one of pre-selected 2048 directions in the transmitting pulse-to-pulse basis. Success of the MU radar in the atmospheric/ionospheric research is well known, and its active phased-array configuration was followed by many other radar systems. The phase control of the MU radar is realized by the control of its transceiver-module (TR-module) that are equipped with each Yagi antenna. They are gathered into 25 groups of each 19 modules. One CPU (microcomputer board) is used for control of one group of modules. A weak point of the MU radar exists in this point because we are using the original 8085 CPU board that is connected to the host computer by 1200-baud (!) serial line. This control is very slow, and we could not meet demands for rapid change of observation parameters for long time. This time we tried to re-develop the new TR-module controller by using recent CPU board and electronic devices. In the presentation, we show hardware/software of the newly developed prototype of the MU radar TR-module controller.