JpGU-AGU Joint Meeting 2020

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] 大気圏ー電離圏結合

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)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Yue Deng(University of Texas at Arlington)、Loren Chang(Institute of Space Science, National Central University)

[PEM12-10] 磁気リップルと電子密度の波状構造およびGPS-TEC変動の空間的・時間的関係

*家森 俊彦1青山 忠司1横山 佳弘1山田 彬泰1 (1.京都大学)

キーワード:磁気リップル、電子密度の波状構造、GPS-TEC変動、重力音波

Wavy structures of electron density (Ne) and magnetic ripples observed along the orbit of Swarm satellites in low-latitude on the dayside, and GPS-TEC variation under the orbit are analyzed to see their correlation. Their apparent periods are typically 20-30 seconds, 10-20 seconds and a few minutes, respectively. Near the equatorial region, the APEX latitudes of the region where wavy Ne structure appears and the region traced down from magnetic ripples to 120km altitude, i.e., ionospheric current layer, often coincide suggesting acoustic mode waves as a common source of their generation. Assuming the GPS-TEC variation with a period around a few minutes is temporal variation, we try to check the correlation in the location among the three quantities to check the validity of our idea that the acoustic mode waves are the common source of the variations.