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astro-ph.SR2026
Testing the 3-equation Kuhfuss Convection Model using the Sun
T. A. M. Braun, F. Ahlborn, F. Kupka +1
Simplified, one-dimensional models are necessary to model convection in the context of stellar evolution. By including the non-local effects of convection, turbulent convection mod…
astro-ph.SR2026★ 1 cited
Third order correlations and skewness in convection. I. A new approach suitable for three-equation non-local models
F. Kupka
Non-local models of stellar convection can account for mixing effects in regions adjacent to convectively unstable layers and for changes to the mean temperature structure caused b…