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Mg ii h&k spectra of an enhanced network region simulated with the MURaM-ChE code. Results using 1.5D synthesis
P. Ondratschek, D. Przybylski, H. N. Smitha +3
The Mg ii h&k lines are key diagnostics of the solar chromosphere. They are sensitive to the temperature, density, and non-thermal velocities in the chromosphere. The average Mg ii…
Jacobian-Free Newton-Krylov method for multilevel NLTE radiative transfer problems
D. Arramy, J. de la Cruz Rodríguez, J. Leenaarts
The calculation of the emerging radiation from a model atmosphere requires knowledge of the emissivity and absorption coefficients, which are proportional to the atomic level popul…
Improved reconstruction of solar magnetic fields from imaging spectropolarimetry through spatio-temporal regularisation
Jaime de la Cruz Rodríguez, Jorrit Leenaarts
Determination of solar magnetic fields with a spatial resolution set by the diffraction limit of a telescope is difficult because the time required to measure the Stokes vector wit…