Turbulent eddy-time-correlation in the solar convective zone
Theoretical modeling of the driving processes of solar-like oscillations is a powerful way of understanding the properties of the convective zones of solar-type stars. In this framework, the description of the temporal correlation between turbulent eddies is an essential ingredient to model mode amplitudes. However, there is a debate between a
Belkacem, K. et al.
Fecha de publicación:
11
2010