日本地球惑星科学連合2023年大会

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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-EM10] Dynamics of Magnetosphere and Ionosphere

2023年5月24日(水) 13:45 〜 15:00 101 (幕張メッセ国際会議場)

コンビーナ:藤本 晶子(九州工業大学)、家田 章正(名古屋大学 宇宙地球環境研究所)、佐藤 由佳(日本工業大学)、今城 峻(京都大学大学院理学研究科附属地磁気世界資料解析センター)、座長:吹澤 瑞貴(国立極地研究所)、佐藤 由佳(日本工業大学)

13:45 〜 14:00

[PEM10-06] F-region depletion in the polar cap ionosphere under quiet geomagnetic conditions

*Khan-Hyuk Kim1、Dong-Hee Kim1、Hyuck-Jin Kwon2、Geonhwa Jee2、Young-Bae Ham2、Changsup Lee2、Jeong-Han Kim2 (1.School of Space Research, Kyung Hee University、2.Korea Polar Research Institute)

キーワード:F-region ionosphere, Polar cap, Polar hole

F-region electron density depletion observed in the winter/nighttime polar cap ionosphere during solar minimum is studied using measurements made from VIPIR/Dynasonde at Jang Bogo Station (JBS), located at Terra Nova Bay in Northern Victoria Land in Antarctica (geographic: 74.62°S, 164.22°E/AACGM geomagnetic: 79.9°S, 53.6°W). We focus on F-region depletion (known as polar hole) events following a steady quiet condition, which is defined with Kp values < 1+ during 6 h. 45 polar holes were identified by JBS VIPIR/Dynasonde in 2019. All of the events started over a wide range of nightside magnetic local time (MLT = 19-03 hr) with a peak occurrence at MLT = 22-24 hr. They ended in a range of MLT = 20-06 hr, and ~82% of them (37 out of 45) ended before 03 MLT, implying that there is a great chance of detecting a polar hole event on the nightside MLT region. The polar hole events last one to five hours. In this study we discuss the role of plasma convection in the formation of the polar holes.