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Development of a High-order Flux Reconstruction Framework for Solar and Astrophysical Magnetohydrodynamics: Methods and Benchmarks
Rayan Dhib et al 2026 The Astrophysical Journal Supplement Series 283 .
Caption: Figure 5.
Evolution of the MHD rotor problem at t = 0.147 (first row) and t = 0.295 (second row), showing pressure field (left) and Mach number (right).
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© 2026. The Author(s). Published by the American Astronomical Society.
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