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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 10.

Line-of-sight velocities of the plasma in different temperature ranges. The emission-measure-weighted mean velocity in the display temperature range is obtained following Equation (6) and is equivalent to the Doppler velocity that would be measured from a spectral line forming in the given temperature range. Positive values (shown in blue) correspond to upflows. The vertical dashed line indicates the slit position for the time–distance diagram shown in Figure 12.

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