日本地球惑星科学連合2014年大会

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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-EM36_28PO1] 大気圏・電離圏

2014年4月28日(月) 18:15 〜 19:30 3階ポスター会場 (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)

18:15 〜 19:30

[PEM36-P26] 日本における50年以上の長期観測データを用いた電離圏嵐統計解析

*中村 真帆1鴨川 仁1 (1.東京学芸大学物理学科)

キーワード:電離圏嵐, foF2, 衛星測位

Statistical analyses of the ionospheric storms over Japan are carried out based on the long-term observations over 50 years in Japan. While there are many types of ionospheric variations such as ionospheric storms, plasma bubbles, TIDs and so on, ionospheric storms are most large fluctuations of electron density in the ionosphere. In general, the increase of the electron density is termed positive storm and the decrease of it is termed negative storm [1]. The positive storms cause satellite-positioning errors due to the delay of radio propagation and negative storms cause HF radio communication outages due to lowering the maximum usable frequency. Because these two types of ionospheric storms shows different characteristics on the duration, scale, and the seasonal dependences, we analyzed ionospheric storm occurrences using critical frequency of the F2 layer; foF2 obtained from ionograms over 4 observation sites (Wakkanai, Kokubunji, Yamagawa, and Okinawa) operated by National Institute of Information and Communications Technology, Japan (NICT) [2]. We extracted ionospheric storms based on the differences between the daily observation values and the one-month median in Japan for more than 50 years. Extracted storms of each station will be analyzed by the occurrences, duration, seasonal dependence and geomagnetic variations.

References
[1] G. W. Prolss, Ionospheric F-region storms, Vol. 2 of Hand book of Atmospheric Electro- dynamics, CRC Press, 1995.
[2] World Data Center for Ionosphere, http://wdc.nict.go.jp/.