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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 6.

A comparison of synthesized EUV emission from run cases on Day 2 with different Ω that adds an additional twist in the magnetic field while keeping the vertical component unchanged (see the main text for details). Each column presents the results from a certain Ω value. The three rows show AIA 171 Å, 131 Å, and 193 Å images, respectively.

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