日本地球惑星科学連合2022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-EM13] Coupling Processes in the Atmosphere-Ionosphere System

2022年5月24日(火) 13:45 〜 15:15 302 (幕張メッセ国際会議場)

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)、コンビーナ:大塚 雄一(名古屋大学宇宙地球環境研究所)、Chang Loren(Institute of Space Science, National Central University)、コンビーナ:Deng Yue(University of Texas at Arlington)、座長:大塚 雄一(名古屋大学宇宙地球環境研究所)、新堀 淳樹(名古屋大学宇宙地球環境研究所)、江尻 省(国立極地研究所)


15:00 〜 15:15

[PEM13-06] Ionospheric irregularities and scintillations during the geomagnetic storm on 15 January 2022

*斎藤 享1吉原 貴之1高橋 透1 (1.国立研究開発法人海上・港湾・航空技術研究所電子航法研究所)

キーワード:電離圏不規則構造、電離圏シンチレーション、地磁気嵐

On 15 January 2022, various ionospheric disturbances were observed over Japan. Some of them appeared to be associated with the volcanic eruption of Hunga Tonga-Hunga Ha'apai. On the other hand, since a moderate geomagnetic storm commenced on 14 January 2022 was going on at the same time, it is important to distinguish the effects of the volcanic eruption and the geomagnetic storm.
We used GNSS total electron contents (TECs) and its temporal fluctuation represented by rate of TEC index (ROTI) derived from GNSS data from GEONET (GNSS Earth Observation Network). Besides the traveling ionospheric disturbances (TIDs) seen in high-pass filtered (detrended) TEC (dTEC) coinciding with atmospheric waves believed to be emitted from the volcanic eruption, multiple band-like regions with ROTI enhancement was started to be observed from 10 UT on 15 January 2022. They extended in the NW-SW direction and apparently moved westward. The structures were not aligned with the TIDs seen in dTEC. In the region of ROTI enhancement, enhancement in TEC was also observed. Stripes of sharp TEC depletions were embedded in the region. This looks similar to the storm-enhanced density (SED) or storm-induced plasma stream (SIPS) observed in the geomagnetic storms.
At the same time, strong scintillation in GNSS signals were observed over Ishigaki Island (24.4N, 124.1E), Japan. A number of TEC depletions embedded in TEC enhancements were observed. Scintillations were observed for almost all the GNSS satellite in view which indicates that the irregularities were distributed over a wide area.
Although it is still unknown that these ionospheric irregularities were due to the geomagnetic storm or combined effects with other sources, this event is important both for understanding the mechanisms of the ionospheric irregularities and for evaluating their effects on GNSS applications.