Oxygen lines in solar granulation: II. Centre-to-limb variation, NLTE line formation, blends, and the solar oxygen abundance
Context: There is a lively debate about the solar oxygen abundance and the role of 3D models in its recent downward revision. These models have been tested using high-resolution solar atlases of flux and disk-centre intensity. Further testing can be done
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|Source:||Astronomy and Astrophysics|
|01_Pereira_Oxygen_lines_in_solar_2009.pdf||439.61 kB||Adobe PDF||Request a copy|
|02_Pereira_Oxygen_lines_in_solar_2009.pdf||809.52 kB||Adobe PDF||Request a copy|
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