日本地球惑星科学連合2021年大会

講演情報

[E] ポスター発表

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-EM11] Coupling Processes in the Atmosphere-Ionosphere System

2021年6月4日(金) 17:15 〜 18:30 Ch.04

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)、Yue Deng(University of Texas at Arlington)

17:15 〜 18:30

[PEM11-P19] Scintillation Drift Velocity Observed by Closely-Spaced GPS Receivers in Indonesia

*大塚 雄一1、Abadi Prayitno2 (1.名古屋大学宇宙地球環境研究所、2.インドネシア航空宇宙庁)

キーワード:赤道電離圏、GPS、プラズマバブル

To investigate zonal drift velocities of a few hundred meter-scale irregularities associated with equatorial plasma bubbles, we have operated three single-frequency GPS receivers at the Equatorial Atmosphere Radar (EAR) site at Kototabang, West Sumatra, Indonesia (0.20oS, 100.32oE; geomagnetic latitude 10.6oS) since January 2003.The GPS receivers sampled GPS signal intensity at a rate of 20 Hz. Distances between the receivers were 116, 127, and 152 m. Drift velocities of irregularities were measured using cross-correlation analysis with the time series of the GPS signal intensity obtained from the three receivers. By analyzing the drift velocity data, equinoctial asymmetry of the zonal drift velocity is found. The eastward drift velocity is higher in March Equinox than in September equinox (Otsuka et al. 2006, Abadi et al., 2017). By analyzing the drift velocity data obtained during a period from 2003 to 2021, in this study, we investigate seasonal and solar activity and magnetic activity dependence of the drift velocity.