Comparing mean-models of different stars

• Horisontal and temporal averages on timescale long compared to p-mode period.
• Horisontal averaging performed on a density-scale (Lagrangian average) to filter out the p-modes.
• Only averaging on relaxed simulations: constant flux, low p-mode amplitude, and no overall movement of the simulation-box.
• Also average quantities seperated in upflows and downdrafts.

• Velocities (macro turbulence)
• Super adiabatic gradients
• Turbulent pressure
• -relations