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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 5.

Histograms of the observed and synthesized intensities in four AIA channels, which are shown in Figure 4. For each channel, the histogram is calculated for the logarithmic intensity and normalized to the numbers of pixels/grid points in the observed/synthesized images. Note that the model-synthesized intensity may contain arbitrarily small numbers. A lower bound is applied to each channel as indicated by the axis.

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