日本地球惑星科学連合2021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-EM13] 太陽地球系結合過程の研究基盤形成

2021年6月4日(金) 17:15 〜 18:30 Ch.05

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)

17:15 〜 18:30

[PEM13-P02] Development of instruments for dual-band beacon (DBB) experiment of total electron content (TEC)

*山本 衛1 (1.京都大学生存圏研究所)

キーワード:デジタル無線技術、全電子数、観測ロケット、2周波数ビーコン

asurement of total electron content (TEC). We are measuring the TEC by using dual-band beacon (DBB) technique. It is to transfer two radio signals at coherent but different frequencies. In the ionospheric plasma, the radio wave's propagation velocity is related to the frequency. By detecting the phase variation between two signals, we can estimate TEC through the radio propagation path. Conventional DBB experiments were carried out using the DBB transmitter on the low Earth orbit (LEO) satellites and receivers on the ground. The most commonly used frequencies are 150MHz and 400MHz. We developed GNU Radio Beacon Receiver (GRBR), the digital receiver, based on the software-defined radio technology. Our new development is the digital receiver GRBR-2, which measures the new beacon signal (401MHz/966MHz) from FORMOSAT-7/COSMIC-2 satellites launched in 2019. Observations with GRBR-2 have already been continued in Indonesia, Thailand, and Vietnam since September 2019. The DBB experiment were also conducted from sounding rockets to the ground. For the new rocket experiment planned in 2022, we are now developing a DBB transmitter and antennas on board of the rocket. On the other hand, recently, TEC observations using Global Navigation Satellite System (GNSS) signals become very popular. While the deployment of GNSS by USA, China, Russia, and the EU progress, the price of receivers have dropped dramatically. This situation helps us to develop a new GNSS-TEC receiver system for multiple-point measurements of the ionospheric. In the lecture we will discuss the current status of our developments.