日本地球惑星科学連合2023年大会

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[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-EM10] Dynamics of Magnetosphere and Ionosphere

2023年5月24日(水) 10:45 〜 12:00 101 (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:北村 成寿(名古屋大学 宇宙地球環境研究所)、藤本 晶子(九州工業大学)

11:45 〜 12:00

[PEM10-05] Statistical analysis of Convection Reversal Boundaries (CRBs) using long-term ion drift observations from DMSP satellite

*Yanshi Huang1、Dongdong Zhao1 (1.Harbin Institute of Technology, Shenzhen)

キーワード:Convective reversal boundary, DMSP satellite, High-latitude ionosphere, Statistical analysis

A new Convection Reversal Boundary (CRB) identification method is investigated using the high-resolution data of Defense Meteorological Satellite Program (DMSP) F16 satellite from the Madrigal website, in order to accurately and effectively identify high-latitude CRBs in both two-cell and multi-cell convection pattern modes. The improved CRB identification method is applied to the ion drift velocity data observed by DMSP F16 satellite from year 2004 to 2015. A long-term statistical study is carried out on these identified CRBs. During the 12 years analyzed in this study, a total of 17,246 CRBs are found, among which majority of them are in the summer and fall seasons during the ascending phase of solar activity. The results demonstrate that the latitudinal distributions of the CRBs in both hemispheres are generally consistent. It is also found that with the enhancement of the solar wind dynamic pressure, the energy coupling function, and the geomagnetic activity, CRBs tend to move more equatorward. With the increasing energy coupling function, the radius of the open magnetic field line region defined by CRBs saturates at about 20° magnetic latitude.