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)
