activity
20112026
most cited3-D non-LTE radiative transfer effects in Fe I lines: II. Line formation in 3-D radiation hydrodynamic simulations

50 citations · 184 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum

Cis Lagae, Ginger Frame, Heather M. Cegla +5

Detecting the radial velocity signal of Earth-mass exoplanets requires the characterisation and removal of granulation-induced radial velocity variability from spectroscopic observ…

astro-ph.SR2025★ 1 cited

Three-dimensional non-LTE radiative transfer effects in Fe I lines IV. Line formation at high spatial resolution

R. Holzreuter, H. N. Smitha, S. K. Solanki

In the first three papers of this series, we investigated the formation of photospheric neutral iron lines in different atmospheres ranging from idealised flux tube models to compl…

astro-ph.SR2021★ 17 cited

Influence of NLTE effects in Fe I lines on inverted atmosphere II. 6301 A and 6302 A lines formed in 3DNLTE

H. N. Smitha, R. Holzreuter, M. van Noort +1

This paper forms the second part of our study on how the neglect of NLTE conditions in the formation of Fe I 6301.5 A and the 6302.5 A lines influences the atmosphere obtained by i…

astro-ph.SR2020★ 33 cited

The influence of NLTE effects in Fe I lines on an inverted atmosphere I. 6301 A and 6302 A lines formed in 1D NLTE

H. N. Smitha, R. Holzreuter, M. van Noort +1

Ultraviolet over-ionisation of iron atoms in the solar atmosphere leads to deviations in their level populations from the Saha-Boltzmann statistics. This causes their line profiles…

astro-ph.SR2015★ 26 cited

3-D non-LTE radiative transfer effects in Fe I lines: III. Line formation in magneto-hydrodynamic atmospheres

René Holzreuter, Sami K. Solanki

Non-local thermodynamic equilibrium (NLTE) effects in diagnostically important solar Fe I lines are important due to the strong sensitivity of Fe I to ionizing UV radiation, which…

astro-ph.SR2013★ 50 cited

3-D non-LTE radiative transfer effects in Fe I lines: II. Line formation in 3-D radiation hydrodynamic simulations

R. Holzreuter, S. K. Solanki

We investigate the effects of horizontal radiative transfer (RT) a NLTE on important diagnostic iron lines in a realistic 3-D HD simulation. Using a multi-level atom we compute and…

astro-ph.SR2012★ 38 cited

Three-dimensional non-LTE radiative transfer effects in Fe I lines I. Flux sheet and flux tube geometries

R. Holzreuter, S. K. Solanki

In network and active region plages, the magnetic field is concentrated into structures often described as flux tubes (FTs) and sheets (FSs). 3-D radiative transfer (RT) is importa…

astro-ph.SR2011★ 19 cited

Observations of the forward scattering Hanle effect in the Ca i 4227 Å line

M. Bianda, R. Ramelli, L. S. Anusha +6

Chromospheric magnetic fields are notoriously diffcult to measure. The chromospheric lines are broad, while the fields are producing a minuscule Zeeman-effect polarization. A promi…