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Table · dataset · 2023

CLV curves of 10 spectral lines taken with SST

Listed in IVOA Registry (Virtual Observatory)

Observations of center-to-limb variations (CLV) of spectral lines and continua provide a good test for the accuracy of models of solar and stellar atmospheric structure and spectral-line formation.

Description

They are also widely used to constrain elemental abundances and are becoming increasingly important in atmospheric studies of exoplanets. However, only a few such data sets exist for chromospheric lines.

We aim to create a set of standard profiles by means of mosaics made with the CRISP and CHROMIS instruments of the Swedish 1-m Solar Telescope (SST), as well as to explore the robustness of said profiles obtained using this method. For each spectral line we use a mosaic that ranges from the center to the limb. Each of these mosaics are averaged down to 50 individual spectral profiles, spaced by 0.02 in the {mu} scale.

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These profiles are corrected for p-mode oscillations, and their line parameters (equivalent width, line shift, full-width at half-maximum, and line depth) are then compared against literature values where possible. We present a set of 50 average profiles that are spaced equidistantly along the cosine of the heliocentric angle ({mu}) by steps of 0.02 for five continuum points between 4001 and 7772{AA}, as well as ten of the most commonly observed spectral lines at the SST (CaII H & K, H{beta}, MgI 5173{AA}, CI 5380{AA}, FeI 6173{AA}, FeI 6301{AA}, H{alpha}, OI 7772{AA}, and CaII 8542{AA}).

Center-to-limb variation of line profiles and continua are shared in the CDS as machine-readable tables, providing a quantitative constraint on theoretical models that aim to model stellar atmospheres.

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Astronomical sciences 69%
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/671/a13013 d agoJSON v1
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