日本地球惑星科学連合2025年大会

講演情報

[J] ポスター発表

セッション記号 S (固体地球科学) » S-EM 固体地球電磁気学

[S-EM16] 地磁気・古地磁気・岩石磁気・環境磁気

2025年5月25日(日) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

コンビーナ:川村 紀子(海上保安大学校 基礎教育講座)、加藤 千恵(九州大学比較社会文化研究院)

17:15 〜 19:15

[SEM16-P19] Eigen mode analysis of the geomagnetic main field: implication to the secular variation evolution

*Hao Luo1 (1.Institute of Geology and Geophysics, Chinese Academy of Sciences)

キーワード:geomagnetic secular variation, eigen mode analysis

The slow temporal variations in Earth’s magnetic field, namely the geomagnetic secular variation (SV), originate in the liquid outer core. The temporal and spatial characteristics of the geomagnetic SV provide vital information for the geomagnetic field evolution and the Earth’s core dynamics. We study the temporal and spatial characteristics by presenting the eigen mode analysis of the geomagnetic main field based on the COV-OBS.x2 model. We found that the geomagnetic SV has obviously regional characteristics. The Pacific region is a region with stable magnetic field structure and slow change, which can be basically represented by the first eigenmode. The northern, central and southern parts of the Atlantic Ocean belong to different eigenmodes and have different characteristics of secular variation. The Indian Ocean is a region with significant and complex changes, and almost every eigenmode has a certain contribution. The intensity of each eigen mode has its own unique period. The small-scale magnetic anomaly corresponds to the short period, while the large scale magnetic anomaly corresponds to the long period. The non-dipole fields are a synthesis of several eigenmodes.