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30日(木) 09:00 〜 10:15 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:Thomas J Immel(University of California Berkeley)、大塚 雄一(名古屋大学宇宙地球環境研究所)

09:00 〜 09:15

[PEM12-01] A-I coupling: Planetary waves driven variability in equatorial plasma bubbles

★Invited Papers

*Ercha Aa1 (1.Haystack Observatory, Massachusetts Institute of Technology)

キーワード:Equatorial Plasma Bubbles (EPBs), Day-to-day variability, Planetary Waves, Atmosphere-Ionosphere coupling

A significant portion of the ionospheric variability can be driven by lower atmospheric forcing such as planetary waves via vertical coupling processes, especially in the equatorial and low-latitude regions. Equatorial plasma bubbles (EPBs) are irregular plasma density depletions that frequently occur in the nighttime equatorial and low-latitude ionosphere. EPBs and associated irregularities can cause satellite signal scintillations and even signal loss of lock, thereby imposing severe space weather effects on communication and navigation systems. However, understanding of the complicated day-to-day variability of EPBs and their connection with lower atmospheric forcing remain a challenging issue for the space weather community. In this study, we use multi-instrument observations (GOLD, ICON, ionosonde) and the WACCM-X simulations to investigate the day-to-day variability of EPBs and to examine their potential connection with planetary waves through the modulation of the Rayleigh-Taylor instability growth rate. Our findings provide new insights into the variability of the ionosphere and its connection with atmospheric waves.