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Coronal Mass Ejections (CMEs) are large-scale eruptions of plasma and magnetic fields from the Sun, capable of impacting Earth’s magnetosphere and triggering geomagnetic storms. These storms can disrupt navigation systems, satellites, and power grids. This study develops a modeling framework using the Community Coordinated Modeling Centre (CCMC) to simulate CME propagation and interactions with Earth’s magnetosphere. We analyze a CME observed during Carrington Rotation 2165 of Solar Cycle 24, emphasizing the importance of continuous observation and advanced modeling in enhancing space weather forecasting.

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A Framework for Studying the Dispersion of CMEs

  • 会议论文

  • 发表日期：

    2025年

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  • Ritesh Sharma,
  • Venktesh Singh,
  • B. Hariharan

摘要

Coronal Mass Ejections (CMEs) are large-scale eruptions of plasma and magnetic fields from the Sun, capable of impacting Earth’s magnetosphere and triggering geomagnetic storms. These storms can disrupt navigation systems, satellites, and power grids. This study develops a modeling framework using the Community Coordinated Modeling Centre (CCMC) to simulate CME propagation and interactions with Earth’s magnetosphere. We analyze a CME observed during Carrington Rotation 2165 of Solar Cycle 24, emphasizing the importance of continuous observation and advanced modeling in enhancing space weather forecasting.