The Solar oxygen abundance as derived using MHD atmospheric models

Damian Fabbian (Instituto de Astrofísica de Canarias, Spain)

We present our initial results on the re-determination of the solar chemical composition using 3D photospheric models that include magnetic fields, a method for the first time employed in determining  the Sun’s oxygen content.

Contributed talk given at the meeting “Mapping Oxygen in the Universe“, Tenerife, Spain (14-18 May 2012)

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