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-EM12] Space Weather and Space Climate

2019年5月28日(火) 15:30 〜 17:00 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:片岡 龍峰(国立極地研究所)、Antti A Pulkkinen(NASA Goddard Space Flight Center)、草野 完也(名古屋大学宇宙地球環境研究所)、坂口 歌織(情報通信研究機構)

[PEM12-P23] Calculating propagation time of HF radio wave using ray-tracing method and simple comparison with the observation.

*中尾 亮1中田 裕之1大矢 浩代1鷹野 敏明1穂積 コンニャナット2津川 卓也2斎藤 享3石井 守2 (1.千葉大学大学院融合理工学府基幹工学専攻電気電子工学コース、2.情報研究通信機構、3.電子航法研究所)

To provide the information of nowcast of radio propagation, we have started a project, HF-START (HF simulator Targeting for All user's Regional Telecommunications). In this project, a simulator that is able to predict propagation of HF radio waves is constructed by ray-tracing calculation.
Using this simulator, we have examined whether HF radio wave travels between any two points. In this calculation, the electron density, which is necessary to calculate reflection index is determined by International Reference Ionosphere (IRI).In this project, HF receivers have been installed at Chiba University (Chiba, 35.62N, 140.10E), Sarobetu (Hokkaido, 45.16N, 141.74E), Numata (Gunma, 36.62N, 139.02E), Yamagawa (Kagoshima, 31.20N, 130.61), Ogimi (Okinawa, 26.68, 128.15E) for observing HF radio wave transmitted from radioNIKKEI (Nagara, Chiba, 35.46N, 140.20E) to confirm the results of the ray-tracing calculation. In the ray-tracing calculation, therefore, we set the same locations of the transmitter and receivers as the observatories of HF-START. As a result of simple comparison between the ray-tracing results and the observation, it is found that there was a difference of the propagation time between the ray-tracing results and the observations. It is possible that the radio wave propagation between radioNIKKEI and Ciba University is not ground wave but sky wave that is reflected by ionosphere. As for further calculation, we plan to use the electron density distributions determined by GAIA and GNSS tomography in the ray-tracing calculation.