JpGU-AGU Joint Meeting 2020

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-EM12] 大気圏ー電離圏結合

コンビーナ:Huixin Liu(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Yue Deng(University of Texas at Arlington)、Loren Chang(Institute of Space Science, National Central University)

[PEM12-33] Development of new receiver for HF Doppler sounding utilized by Software-Defined Radio device

*中田 裕之1大木 悠平2野崎 憲朗3細川 敬祐3冨澤 一郎3松嶋 諒3橋本 久美子4鷹野 敏明1大矢 浩代1 (1.千葉大学大学院工学研究院、2.千葉大学工学部電気電子工学科、3.電気通信大学、4.吉備国際大学)

キーワード:HFドップラー観測、受信機開発、ソフトウェア無線、USRP

To examine the dynamics of the ionosphere, the observation of both steady and disturbed states of the ionosphere is important. Various observation systems have been utilized to observe the behaviors of the ionosphere itself and the ionospheric disturbances. One of the useful observation systems is HF Doppler sounding. When the reflection point of the radio wave moves vertically, the frequency of the radio wave shifts due to the Doppler effect. From this Doppler frequency, we are able to estimate the vertical motions of the ionospheric plasma. To develop and maintain the transmitter and the receiver of Doppler sounding system, the knowledge of the analog circuit has been inevitable. Recently, on the other hand, Software-Defined Radio (SDR) device, which equips digital electronics for signal processing, is developed and make it possible to develop the equipments for HF Doppler sounding system easily by utilizing the software processing. This means that the receivers for HF Doppler sounding system are developed without the knowledge of the analog circuits. Therefore, we have developed the new HF receiver using SDR device instead of the traditional receiver. In this study, we adopted USRP N210 as a new SDR device. In HFD sounding system, the transmitter for 5.006 MHz and 8.006 MHz is located at Chofu Campus of the University of Electro-Communications and that for 6.055 MHz and 9.595 MHz (now off the air) is Radio NIKKEI transmitter located at Nagara. The previous receiver can observe radio waves at four different frequencies with 100 Hz sampling. New SDR receiver is also enable to observe the four different radio waves with 160 Hz sampling. Test observation of the new SDR receiver were performed in Awaji with the previous receiver. We compared the observational results of Doppler frequencies between both receivers.
The Doppler frequencies of the sky wave observed by SDR receiver and the previous analog receiver are coincided each other. Therefore, it is found that the new receiver can be utilized for the actual observation. New SDR receivers will be installed at Onna, Sarobetsu, and existing stations.