Donghui Son

PhD Candidate in Solar Physics
Kyung Hee University

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Parker Instability Aug 4, 2024

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Emerging flux tube
Shock Speed Derivation
What determines the brightness of magnetically open solar corona?: Insights from three-dimensional radiative MHD simulations and observations (Iijima, H., 2025)
Convective Magnetic Flux Emergence Simulations from the Deep Solar Interior to the Photosphere: Comprehensive Study of Flux Tube Twist (Toriumi, S., 2024)
L5 지점 관측의 한계와 전망: 우주기상 예보 패러다임의 전환

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