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Time-dependent Three-dimensional MHD Simulation of Solar Corona and Solar Wind at Solar Minimum Activity Phase

Keiji Hayashi, Y. Liu, X. P. Zhao

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Key concepts: Corona (planetary geology), Coronal mass ejection, Solar wind, Nanoflares, Magnetohydrodynamics, Atmospheric sciences, Physics, Solar cycle 22

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Time-dependent Three-dimensional MHD Simulation of Solar Corona and Solar Wind at Solar Minimum Activity Phase — Research Paper | ScholarLens