2 papers
astro-ph.SR2021
Non-equilibrium Equation of State in stellar atmospheres
L. S. Anusha, M. van Noort, R. H. Cameron
In the stellar chromospheres, radiative energy transport is dominated by only the strongest spectral lines. For these lines, the approximation of local thermodynamic equilibrium (L…
astro-ph.SR2020
Power spectrum of turbulent convection in the solar photosphere
L. Yelles Chaouche, R. H. Cameron, S. K. Solanki +15
The solar photosphere provides us with a laboratory for understanding turbulence in a layer where the fundamental processes of transport vary rapidly and a strongly superadiabatic…