日本地球惑星科学連合2018年大会

講演情報

[EE] 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-EM13] 太陽地球系結合過程の研究基盤形成

2018年5月20日(日) 09:00 〜 10:30 304 (幕張メッセ国際会議場 3F)

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、共同)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)、座長:山本 衛野澤 悟徳

09:15 〜 09:30

[PEM13-02] Development of Software-Defined Multi-Channel Receiver System for the Equatorial Atmosphere Radar (EAR)

*Nor Azlan Bin Mohd Aris1,2Hiroyuki Hashiguchi1Mamoru Yamamoto1 (1.Research Institute for Sustainable Humanosphere、2.Universiti Teknikal Malaysia Melaka)

キーワード:VHF radar, Multi-channel receiver, USRP, GNU Radio

Equatorial Atmosphere Radar (EAR) was established in June 2001 by the collaboration between Research Institute for Sustainable Humanosphere (RISH), Kyoto University and Indonesian National Institute of Aeronautics and Space (LAPAN). EAR is a VHF Doppler radar operated at 47 MHz with an active phased-array antenna system and located at the equator at Kototabang, West Sumatra, Indonesia (0.20oS, 100.32oE, 865 m above sea level). Established with a single receiving channel until currently, here we present the development of multi-channel receiver system for the EAR using the combination of Universal Software Radio Peripheral X300 (USRP X300) series and GNU Radio. Two USRP X300 devices corresponding to four receiving channels are synchronized using 10 MHz reference clock and 1 pulse per second (PPS) signal. Received signals are collected by the existing EAR antennas and fed to the USRPs for digital conversion and then stored in Hard Disk Drive (HDD). Signals post-processing are carried out to obtain the Doppler spectra and the measurement of wind speed and direction.