日本地球惑星科学連合2024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-EM12] Coupling Processes in the Atmosphere-Ionosphere System

2024年5月30日(木) 17:15 〜 18:45 ポスター会場 (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)

17:15 〜 18:45

[PEM12-P29] Classification of Ionograms in the Polar region by the Vertical Incidence Pulsed Ionospheric Radar at Jang Bogo Station, Antarctica

*Junho Back1,2、Geonhwa Jee2,3、Hyuck-Jin Kwon2Khan-Hyuk Kim1、Changsup Lee2,3、Young-Bae Ham2,3 (1.School of Space Research, Kyung Hee University、2.Division of Atmospheric Sciences, Korea Polar Resarch Institue、3.Department of Polar Scienc, Korea University of Science and Technology)

キーワード:Ionogram

The electron density profile of an ionogram is traditionally estimated using image processing techniques based on the shape of echoes reflected in the ionosphere. Vertical Incidence Pulsed Radar (VIPIR) with Dynasonde, however, uses a 3-D inversion program named NeXtYZ, which estimates the electron density profile through phase analysis of reflected echoes. In this study, we automatically classified ionograms obtained from VIPIR/Dynasonde installed at Jang Bogo Station (JVD) for a 5-year period from 2017 to 2021 to validate the efficiency of the NeXtYZ program. We found that more than 50% of ionograms show a reasonable electron density profile. However, NeXtYZ did not properly calculate electron density profiles under dynamic structures of the polar ionosphere, such as sporadic-E and aurora. The distribution of good profiles depends on magnetic local time and season, which may be attributed to the effects of solar irradiation and electric fields at high latitudes. In future work, we will investigate the reasons behind the frequent occurrence of Es layers during the winter seasons and in the dawn and dusk sectors.