日本地球惑星科学連合2024年大会

講演情報

[E] 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-EM15] 太陽地球系結合過程の研究基盤形成

2024年5月29日(水) 10:45 〜 12:15 展示場特設会場 (2) (幕張メッセ国際展示場 6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)、座長:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)

11:15 〜 11:30

[PEM15-03] Latest activities of i-SPES & Kyutech FM-CW project: 2023

*藤本 晶子1阿部 修司2吉川 顕正2池田 昭大3、廣重 優1、中村 駿仁1、牛王 悠輝1 (1.九州工業大学、2.九州大学、3.鹿児島工業高等専門学校)

キーワード:電離圏観測

The ionosphere, from about 100km to high altitudes, has a significant impact on the radio propagation for communications, satellite positioning system, etc. The structure of ionosphere is not stable and variable in the time of day, season, latitude, and solar activity, because of the differences of the energetic photo-ionization process. The irregularities and disturbances in the ionosphere cause various severe problems, for example, lower accuracy of the radio navigation due to the global positioning system/Global Navigation Satellite System scintillation, disruptions in High Frequency (HF) radio wave bands or interferences due to anomalous propagation, etc. To utilize radio propagation safely and securely in modern society, it is essential to measure and analyze the fluctuating ionospheric environment at high speed and with high accuracy.

An FM-CW (Frequency Modulated Continuous Wave) radar is a type of HF (High Frequency) radar. We have installed and operated four FM-CW stations along the Japanese longitude, in Japan, Russia, Philippine, and Peru, to measure the electric fields penetrating the ionosphere. We have been developing the SDR (Software-Defined Radio)-based scintillation detector system integrated with FM-CW and MAGDAS (http://data.icswse.kyushu-u.ac.jp) projects. In this paper, we will present the following latest activities of our project: proposal of a new detection method of Ionogram echoes and latest status of development of software radio-GPS scintillation measurements.