日本地球惑星科学連合2023年大会

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[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-EM09] Space Weather and Space Climate

2023年5月26日(金) 15:30 〜 17:00 101 (幕張メッセ国際会議場)

コンビーナ:片岡 龍峰(国立極地研究所)、Antti A Pulkkinen(NASA Goddard Space Flight Center)、Mary Aronne中村 紗都子(名古屋大学宇宙地球環境研究所)、座長:片岡 龍峰(国立極地研究所)、Antti A Pulkkinen(NASA Goddard Space Flight Center)

16:45 〜 17:00

[PEM09-27] Validation of HF Radio attenuation calculation using HF Doppler observation

佐藤 駿1、*中田 裕之2穂積 コンニャナット3斎藤 享4細川 敬祐5大矢 浩代2 (1.千葉大学大学院融合理工学府、2.千葉大学大学院工学研究院、3.情報通信研究機構、4.海上・港湾・航空技術研究所 電子航法研究所、5.電気通信大学)

キーワード:HF帯電波、減衰、レイトレーシング、HFドップラー

Since the ionospheric conditions for radio wave propagation change diurnally and seasonally, the accurate estimation of the current state of radio wave propagation would be very useful. We have already developed the web service providing the propagation paths of HF radio waves as part of the HF-START (HF Simulator Targeting for All users’ Regional Telecommunications) project. On the other hand, actual radio waves are attenuated by various causes, and the signal intensity varies depending on the ionospheric conditions and propagation path. Therefore, in addition to the propagation paths, it is quite helpful to estimate the signal intensity of radio waves.
To provide information on the signal intensity, we have developed a calculator to determine the attenuation of HF radio waves in the ionosphere. The main factors for the attenuation of HF radio waves are (1)particle collisions in the ionosphere, (2)ground reflection, and (3) free space loss. In this study, the attenuation due to particle collisions in the ionosphere was estimated simultaneously with the raytracing calculation of the propagation paths. The absorption coefficient of the radio wave was adopted from that defined by Davies (1990).
We compared the temporal variation of the signal intensity of the o-mode radio wave with those observed by HF Doppler Sounding. In this comparison, we set the transmitting and receiving points as Chofu Campus (at the University of Electro-Communications 35.657N, 139.543E) and Sugadaira (36.423N, 138.318E), respectively. The frequency of the radio waves was 5.006 MHz. As a result, the dependences of daily and seasonal variations on the signal intensity were very similar between the simulation and the observations: the signal intensity decreased during the daytime and summer when the electron density was large. This result also implies that the propagation mode of HF Doppler Sounding between Chofu and Sugadaira is o-mode. These results suggest that the estimation of the absorption in this study helps estimate the realistic signal intensity for propagation between any two points on the ground.