The elemental composition of the Sun I. The intermediate mass elements Na to Ca
Pat Scott, Nicolas Grevesse, Martin Asplund, A. Jacques Sauval, Karin, Lind, Yoichi Takeda, Remo Collet, Regner Trampedach, Wolfgang Hayek

TL;DR
This paper presents a highly detailed re-evaluation of the Sun's intermediate-mass element composition (Na to Ca) using advanced 3D hydrodynamic models, providing more accurate and systematic abundance measurements than previous studies.
Contribution
It introduces a comprehensive 3D+NLTE analysis of solar Na to Ca abundances, improving accuracy and consistency over earlier 1D models, with detailed error analysis and updated data.
Findings
3D+NLTE abundances are systematically lower than previous 1D results.
The $ extless$3D$ extgreater$ model yields similar results to full 3D calculations.
The study provides a detailed, homogeneous set of solar abundances for Na to Ca.
Abstract
The composition of the Sun is an essential piece of reference data for astronomy, cosmology, astroparticle, space and geo-physics. This article, dealing with the intermediate-mass elements Na to Ca, is the first in a series describing the comprehensive re-determination of the solar composition. In this series we severely scrutinise all ingredients of the analysis across all elements, to obtain the most accurate, homogeneous and reliable results possible. We employ a highly realistic 3D hydrodynamic solar photospheric model, which has successfully passed an arsenal of observational diagnostics. To quantify systematic errors, we repeat the analysis with three 1D hydrostatic model atmospheres (MARCS, MISS and Holweger & M\"{u}ller 1974) and a horizontally and temporally-averaged version of the 3D model (3D). We account for departures from LTE wherever possible. We have…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Solar and Space Plasma Dynamics
