日本地球惑星科学連合2024年大会

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] Coupling Processes in the Atmosphere-Ionosphere System

2024年5月31日(金) 10:45 〜 12:00 展示場特設会場 (2) (幕張メッセ国際展示場 6ホール)

コンビーナ:細川 敬祐(電気通信大学大学院情報理工学研究科)、Liu Huixin(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)、Chang Loren(Institute of Space Science, National Central University)、Chairperson:Jia Yue(NASA Goddard Space Flight Center)、Chang Loren(Institute of Space Science, National Central University)

10:45 〜 11:00

[PEM12-26] Recent observations of Atmospheric-Ionospheric coupling and Doppler sounding in Europe

★Invited Papers

*Jaroslav Chum1、Jaroslav Urbář1 (1.Institute of Atmospheric Physics of the Czech Academy of Sciences)

キーワード:Ionosphere, Perturbations, Earthquake, Infrasound, Geomagnetic storm

Continuous Doppler sounding of the ionosphere is a simple and useful tool to investigate and analyze perturbations in the ionosphere on short time scales (including infrasonic periods) caused by forcing from below and above. The application of Doppler sounding will be shown on two examples:
a) Detection and analysis of infrasound waves in the European ionosphere generated by the recent devastating earthquake sequence in Turkey on 6 February 2023. Imprints of seismic P, S and Rayleigh waves were clearly observed in the ionosphere in central Europe for the second M=7.7 shock at 10:24 UT. Using observation and simulation, it is discussed that infrasound of a given frequency can only reach specific heights due to attenuation. In the studied case, the infrasound frequency was around 0.05 Hz (period ~20 s) and the waves were attenuated above ~200 km. Thus, the ionospheric co-seismic signatures were only detected for the daytime M=7.7 earthquake that occurred at 10:24 UT (11:24 LT in Czechia), but not for the nighttime M=7.8 earthquake that took place about 9 hours before at 01:17 UT, when the ionosphere was much thinner and sounding signals reflected at altitudes larger than 300 km.
b) Ionospheric disturbances observed during the geomagnetic storm on 5 November 2023 that caused large perturbations of electron densities and movement of ionospheric plasma. The ionospheric fluctuations are compared with local geomagnetic data and solar wind forcing. In addition, the effect on GNSS accuracy is presented. Regional differences between ionospheric perturbations in Belgium, Czechia and Slovakia are also shown.