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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 1.

Comparison between the observed vertical magnetic field and the vertical magnetic field (Bz) in the zero-β model. The field of view covers the main sunspots in the active region. The top row presents the observed magnetic field with grayscale saturation at ±1000 G. The middle row shows Bz in the first layer in the computational domain. The bottom row compares the observed Bz and that in the data-driven model along the blue dashed lines, as marked in the top two rows.

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