K-epsilon models of the lower overshoot layer
Apart from the solar core, the overshoot layer below the convective zone is the layer where some discrepancies between the standard and seismic solar models continue to exist. Non-local mixing length models are in clear conflict with the seismic evidence. A major difficulty for the development of more sophisticated models is the large degree of
Petrovay, K.
Fecha de publicación:
0
1998