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.
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2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
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astro-ph.SR 2years
2026 2representative citing papers
Stokes inversions show the Evershed flow reverses to inflow in the upper photosphere while the moat flow remains an outflow, and umbral flashes exhibit supersonic upflows with Mach numbers at least 1.5 consistent with shock fronts.
citing papers explorer
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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.
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Chromospheric and photospheric properties of sunspots as inferred from Stokes inversions under magneto-hydrostatic and non-local-thermodynamic equilibrium
Stokes inversions show the Evershed flow reverses to inflow in the upper photosphere while the moat flow remains an outflow, and umbral flashes exhibit supersonic upflows with Mach numbers at least 1.5 consistent with shock fronts.