Solar Abundance Corrections Derived Through Three-dimensional Magnetoconvection Simulations
We explore the effect of the magnetic field when using realistic three-dimensional convection experiments to determine solar element abundances. By carrying out magnetoconvection simulations with a radiation-hydro code (the Copenhagen stagger code) and through a posteriori spectral synthesis of three Fe I lines, we obtain evidence that moderate
Fabbian, D. et al.
Advertised on:
12
2010