Japan Geoscience Union Meeting 2024

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM12] Coupling Processes in the Atmosphere-Ionosphere System

Thu. May 30, 2024 1:45 PM - 3:00 PM Exhibition Hall Special Setting (2) (Exhibition Hall 6, Makuhari Messe)

convener:Keisuke Hosokawa(Department of Communication Engineering and Informatics, University of Electro-Communications), Huixin Liu(Earth and Planetary Science Division, Kyushu University SERC, Kyushu University), Yuichi Otsuka(Institute for Space-Earth Environmental Research, Nagoya University), Loren Chang(Department of Space Science and Engineering, National Central University), Chairperson:Charles Lin(Department of Earth Sciences, National Cheng Kung University), Keisuke Hosokawa(Department of Communication Engineering and Informatics, University of Electro-Communications)

1:45 PM - 2:00 PM

[PEM12-11] Largest thermospheric wind ever observed with a Fabry-Perot interferometer in Tromsø, Norway since 2009 during the March 2023 storm

*Shin-ichiro Oyama1,2, Heikki Vanhamaki3, Lei Cai3, Atsuki Shinbori1, Keisuke Hosokawa4, Takeshi Sakanoi5, Kazuo Shiokawa1, Anita Aikio3, Ilkka I Virtanen3, Nozomu Nishitani1, Yasunobu Ogawa2, Yoshizumi Miyoshi1, Satoshi Kurita6 (1.Institute for Space-Earth Environmental Research, Nagoya University, 2.National Institute of Polar Research, 3.University of Oulu, 4.The University of Electro-Communications, 5.Planetary Plasma and Atmospheric Research Center, Tohoku University, 6.Research Institute for Sustainable Humanosphere, Kyoto University)

Keywords:thermospheric wind, geomagnetic storm, Fabry-Perot interferometer, ion drag, Joule heating, polar region

Solar cycles 24-25 were quiet until a geomagnetic storm with a Sym-H index of -170 nT occurred in late March 2023. On March 23-24, a Fabry-Perot interferometer (FPI; 630 nm) in Tromsø, Norway, recorded the highest thermospheric wind speed of over 500 m/s since 2009. Comparisons with magnetometer readings in Scandinavia showed that a large amount of electromagnetic energy was transferred to the ionosphere-thermosphere system. Total electron content maps suggested an enlarged auroral oval and revealed that the FPI observed winds near the polar cap instead of inside the oval for a long period during the storm main phase. The FPI wind had a strong equatorward component during the storm, likely because of the powerful anti-sunward ionospheric plasma flow in the polar cap. The positive Y-component of the IMF for six days before the storm caused a successive westward component of the FPI-measured wind during the storm main phase. On March 24, the first day of the storm recovery phase, thermospheric wind disturbed and the ionospheric density decreased significantly at high latitudes. This density depression lasted for several days, and a large amount of electromagnetic energy during the storm modified the thermospheric dynamics and ionospheric plasma density.