Kavli Affiliate: Robert Cameron | Summary:Stellar convection in the presence of magnetic field affects the emergent intensity, as well as the structure and evolution of cool main-sequence dwarfs. We aim to understand the effect of faculae-like field strengths on near-surface stellar convection using 3D radiative MHD simulations of near-surface magneto-convection. We compare simulations of F, […]
Continue.. Simulations of facular magnetic fields on cool stars I: Main sequence stars with solar metallicity