日本地球惑星科学連合2019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-EM09] Vertical coupling in the atmosphere and Ionosphere

2019年5月29日(水) 13:45 〜 15:15 A03 (東京ベイ幕張ホール)

コンビーナ: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)、Chang Loren(Institute of Space Science, National Central University)、大塚 雄一(名古屋大学宇宙地球環境研究所)、座長:Patrick Espy(Norwegian University of Science and Technology)、Astrid Maute(National Center for Atmospheric Research, US)

14:55 〜 15:15

[PEM09-05] Ionospheric Variability Associated with the Quasi-6-day Planetary Wave

★Invited Papers

*山崎 洋介1 (1.ドイツ地球科学研究センター)

キーワード:電離圏/熱圏、準6日波、赤道域

The state of the ionosphere varies from day to day. This is partly due to atmospheric waves that propagate to the upper atmosphere from below. The present study investigates the ionospheric variability associated with the quasi-6-day wave (Q6DW), which is a westward-traveling planetary wave with zonal wave number s=1 and period around t=6d. First, the Q6DW effect on the equatorial ionospheric electric field is examined using the equatorial electrojet measurements from CHAMP and Swarm satellites, as well as ground-based magnetometer and radar observations. Case studies are presented where westward-propagating disturbances with s=1 and t~6d are observed in the daytime equatorial ionospheric electric field. Geopotential height measurements from the Aura satellite confirm the presence of the Q6DW in the lower thermosphere during those events. Next, the impact of the Q6DW on the equatorial ionization anomaly (EIA) is assessed using global maps of total electron content (TEC) from Global Positioning System data. It is shown that the amplitude of the Q6DW in TEC is largest at the EIA crest latitudes and its intra-annual variability closely follows the Q6DW variability in the lower thermosphere.