Mg II h&k spectral line properties computed using 3D radiative transfer in an enhanced network region simulated with the MURaM-ChE code

Open Access

Fig. 1.

Spatially averaged spectra of the Mg II h&k lines. Shown are the spectra from the MURaM-ChE simulation once computed in full 3D RT (red) and once using the plane-parallel 1.5D RT approximation (gray). For comparison, we show an observation from a qualitatively similar bipolar feature, which covers a similar area on the Sun (black).

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