日本地球惑星科学連合2024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-EM11] Space Weather and Space Climate

2024年5月28日(火) 13:45 〜 15:15 展示場特設会場 (2) (幕張メッセ国際展示場 6ホール)

コンビーナ:片岡 龍峰(国立極地研究所)、Aronne Mary(NASA Goddard Space Flight Center)、伴場 由美(国立研究開発法人 情報通信研究機構)、Pulkkinen Antti(NASA Goddard Space Flight Center)、座長:片岡 龍峰(国立極地研究所)、Mary Aronne

14:00 〜 14:15

[PEM11-17] Causality Relationships Analysis in Magnetospheric Space Weather: The Case of the Dst Index and Its Potential Drivers

*Dr Hua-Liang Wei1Michael A Balikhin1、Richard J Boynton1Simon N Walker1 (1.The University of Sheffield)

キーワード:Space weather, Dst index, System identification, Causality analysis

Understanding, quantifying and modelling the response behaviour of the Earth’s magnetosphere to the solar wind is important for evaluating and monitoring the impacts of space weather on our Earth. The analysis and accurate characterization of the causal relationship from solar wind to magnetosphere is difficult because the evolution and response of the associated dynamics are complex, nonlinear and time-varying. In this work, a nonlinear dynamic system identification approach, called Nonlinear Autoregressive Moving Average with eXogenous inputs (NARMAX) method, together with other methods, is applied to investigate Granger causal relationships from solar wind parameters to the intensity of geomagnetic storms characterized by the Dst index. For illustration purposes, causality test results obtained from data of Dst index three solar wind parameters (solar wind velocity, dynamic pressure and proton density), and two interplanetary magnetic field (IMF) indices (southward IMF and solar wind rectified electric field), are presented to show the performance of the proposed causality analysis methods.