3D NLTE sodium abundance corrections relative to 1D LTE are typically negative and larger for saturated lines in giants, reaching -0.7 dex, with a public grid released for use.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
representative citing papers
A forward-modeling technique extracts spatially resolved cavity separation, reflectivities, and prefilter curves for dual-etalon FPI systems from quiet-Sun observations without hardware changes, yielding RMS cavity variation below 2 nm and reflectivity variations of 0.3-0.4% for the CRISP2 camera.
A spatial-variability proxy method applied to MURaM and MPS-ATLAS simulations of the Sun reveals stronger line-strength variations in neutral-element lines and larger central-wavelength shifts in singly-ionized lines.
citing papers explorer
-
3D NLTE Sodium abundances in late-type stars. Abundance corrections and synthetic spectra
3D NLTE sodium abundance corrections relative to 1D LTE are typically negative and larger for saturated lines in giants, reaching -0.7 dex, with a public grid released for use.
-
Characterization of telecentric dual-etalon Fabry-P\'erot systems from observational data. Properties of the CRISP2 instrument at the Swedish 1-m Solar Telescope
A forward-modeling technique extracts spatially resolved cavity separation, reflectivities, and prefilter curves for dual-etalon FPI systems from quiet-Sun observations without hardware changes, yielding RMS cavity variation below 2 nm and reflectivity variations of 0.3-0.4% for the CRISP2 camera.
-
Sensitivity of spectral lines to granulation: The Sun
A spatial-variability proxy method applied to MURaM and MPS-ATLAS simulations of the Sun reveals stronger line-strength variations in neutral-element lines and larger central-wavelength shifts in singly-ionized lines.