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Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code: Coronal Heating and Dynamics in an Emerging Active Region

  • Authors: Feng Chen

Feng Chen 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 9.

Synthesized AIA 171 Å images of the radiative MHD models (on Day 2) with standard and high resolutions. The left column shows the Ω0 and Ω3 models calculated with standard horizontal resolution (512 grid points × 288 km grid spacing). The right column displays the models calculated with the same parameters but a high-resolution mesh (1024 grid points × 144 km grid spacing). The vertical grid spacing for all of the models is 64 km.

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