日本地球惑星科学連合2019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-EM14] Recent Advances in Ionosphere Observation and Modeling for Monitoring and Forecast

2019年5月26日(日) 10:45 〜 12:15 ポスター会場 (幕張メッセ国際展示場 8ホール)

コンビーナ:Yang-Yi Sun(China University of Geosciences)、LIN CHIYEN(Center for Astronautical Physics and Engineering, National Central University, TAIWAN)、MINYANG CHOU(National Cheng Kung University)

[PEM14-P03] The First Result on Ionospheric Space Weather of FORMOSAT-5/AIP Ion Density

*FU-YUAN CHANG1JANN-YENQ Liu1Chi-Kuang Chao1 (1.National Central University)

キーワード:topside ionosphere, equatorial plasma depletion bay, plasma drift

The science payload of Advantage Ionosphere Probe (AIP) onboard FORMOSAT-5 (F5) launched on 24 August 2017 has being operated in a Sun synchronous orbit at 720km altitude with an inclination angle of 98.28 degrees and the revisit period every 2-day. The global distribution of F5/AIP ion density (Ni) in nighttime of 2200LT during November 2017-October 2018 is examined and reported. F5/AIP ion densities show that equatorial plasma depletions frequently appear over South America, Africa, and Asia sectors; four-peaked EIA (non-migrating tide) structures prominently occur in September-March; and plasma depletion bays (PDBs) at low-latitudes in April-August. It is found that prominent locations of the plasma depletions slightly differ from those of equatorial irregularities, while non-migrating tide and PDBs result from different physical mechanisms.