日本地球惑星科学連合2016年大会

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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-EM16] 大気圏・電離圏

2016年5月24日(火) 15:30 〜 17:00 106 (1F)

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:大山 伸一郎(名古屋大学 宇宙地球環境研究所)、横山 竜宏(情報通信研究機構)

16:30 〜 16:45

[PEM16-17] LF帯標準電波を用いた台風に関連する下部電離圏反射高度変動

*大矢 浩代1淺田 圭佑2土屋 史紀3塩川 和夫4中田 裕之1山下 幸三5高橋 幸弘6 (1.千葉大学大学院工学研究科、2.千葉大学工学部、3.東北大学大学院理学研究科、4.名古屋大学宇宙地球環境研究所、5.サレジオ工業高等専門学校電気工学科、6.北海道大学大学院理学研究院)

So far, several studies for gravity waves caused by typhoons have been reported, although there are few studies for the lower ionosphere variations associated with typhoons using LF transmitter signals. In this study, we investigate variations of the D-region height associated with a typhoon of 11-20 June, 2012 using phase data of LF transmitter signals. There were two magnetic storms (minimum Dst values:-51 nT on 12 June and -71 nT on 17 June) in these dates. The propagation paths were Fukushima-Pontianak (PTK, Indonesia, 40 kHz) and Saga-PTK (60 kHz). We converted the phase data to reflection heights based on Earth-ionosphere waveguide mode theory. The period of the reflection height variations was analyzed by wavelet transform. The reference days were 23, 24, and 29 June, 2012, which were also geomagnetically quiet days. We excluded the periods of the reflection height variations seen in these reference days from the periods during the typhoon. In daytime during the typhoon, several solar flares were identified by the GOES X-ray flux. When the solar flares occurred, the reflection heights were largely decreased. Only nighttime data of the reflection height were analyzed because the duration of the gravity waves is expected to be several hours. As a result, the common periods of the reflection height over both propagation paths were 45.3 minutes on 15 June, 2012, and 76.1 minutes on 16 June. The duration of the periods was about 50 minutes in nighttime. In the two nights, medium-scale traveling ionospheric disturbances were not observed in the GPS-TEC data over Japan. The horizontal wavelengths were calculated from the onset time difference of the oscillations between the two propagation paths, and difference of the distance between the source location (the typhoon) and the two propagation paths. The horizontal wavelengths were estimated to be 483 – 662 km for the 45.3 minutes and 1222 – 1346 km for the 76.1 minutes. The horizontal wavelengths were comparable or longer than previous studies.