日本地球惑星科学連合2014年大会

講演情報

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-EM36_28PM2] 大気圏・電離圏

2014年4月28日(月) 16:15 〜 18:00 312 (3F)

コンビーナ:*大塚 雄一(名古屋大学太陽地球環境研究所)、津川 卓也(情報通信研究機構)、川村 誠治(独立行政法人 情報通信研究機構)、座長:松村 充(電気通信大学附属宇宙・電磁環境研究センター)、横山 竜宏(情報通信研究機構)

17:15 〜 17:30

[PEM36-P12_PG] JARE55 南極観測船「しらせ」船上、標準電波強度計測:初期結果報告

ポスター講演3分口頭発表枠

*北内 英章1野崎 憲朗1伊東 宏之1近藤 巧1土屋 茂1今村 國康1長妻 努1 (1.情報通信研究機構)

キーワード:low frequency (LF) radio waves, call sign JJY of 40 kHz and 60 kHz, standard frequency and time signals (SFTS), self calibration, Japanese Antarctic Research Expedition (JARE), Japanese Antarctic Research Icebreaker Shirase

We developed a highly sensitive, reliable receiving system for the purpose of reception of low frequency (LF) radio waves. The system consists of digital lock-in amplifiers and crossed-loop antennas. Digital lock-in amplifier (DLA) employs phase-sensitive detection (PSD) of periodic signal multiplied by the input reference source of the known signal frequency. This makes it possible to realize very narrow bandpass filter around the reference frequency, detecting/measuring that of very weak signal even in noisy environment. The antenna, on the other hand, consists of orthogonally crossed, larger double loops (receivers RX, RY) and smaller doubles (transmitters TX, TY): the former receivers RX, RY receive LF radio signals of x-, y-components, the latter transmitters TX, TY transmit an instant, weak signal from each x-, y-component for self calibration purpose. The self calibration test is performed by transmitting a weak LF signal for an instant every an hour from the transmitter TX, TY respectively, and receiving this signal from the receivers RX, RY to obtain preassigned field strength. This test indicates if the receivers of the system are working properly and allows us to obtain reliable measurements.

We apply the receiving system to measure the field intensity and phase of the standard frequency and time signals (SFTS) JJY of LF 40 kHz and 60 kHz during the summer expedition of the 55th Japanese Antarctic Research Expedition (JARE), from November 2013 to April 2014. Figure 1 shows temporal evolution of the field intensities JJY 40 kHz (light blue dots) and 60 kHz (brown dots) as well as the self-calibrating radio signals. Our receiving system detects both the LF JJY radio signals even offshore Syowa Station, Antarctic, about 14,000 km away from those transmitting stations. Also the field intensities of the self calibration test show about a consistent preassigned value, assuring the measurements.