3D RT in a MURaM-ChE enhanced network simulation produces Mg II h&k lines closer to IRIS data than 1.5D, showing larger 1.5D-3D discrepancies than Bifrost due to horizontal velocities and more scatter in correlations.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2026 1verdicts
ACCEPT 1representative citing papers
citing papers explorer
-
Mg II h&k spectral line properties computed using 3D radiative transfer in an enhanced network region simulated with the MURaM-ChE code
3D RT in a MURaM-ChE enhanced network simulation produces Mg II h&k lines closer to IRIS data than 1.5D, showing larger 1.5D-3D discrepancies than Bifrost due to horizontal velocities and more scatter in correlations.