新鲜 发表于 2025-3-23 10:09:31
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On Solar and Solar-Like Stars Convection, Rotation and Magnetismibutions have impacted or challenged the current state of our understanding and guided the development of advanced numerical simulations of the magnetohydrodynamics (MHD) of the Sun and Sun-like stars.atopic-rhinitis 发表于 2025-3-24 03:42:36
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Writing Patient Education Materialsw ideas. He spent six years in Sheffield after being appointed as the Head of Applied Mathematics Department in the University of Sheffield (UK) where colleagues hold fond memories of him, both as a committed academic and a very effective leader. His hard work and sincere approach was infectious toRankle 发表于 2025-3-24 15:09:48
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Response to Bryan and Beauchampeismic data forthcoming from the GONG, MDI (on SOHO) and HMI (on SDO) observational projects. This has enabled major discoveries about the internal differential rotation of the Sun, revealing both a tachocline of shear at the base of its convection zone and a near-surface shear layer near its surfac