Seismic properties of the Sun's superadiabatic layer .1. Theoretical modelling and parametrization of the uncertainties
Some alternatives to the traditional mixing-length theory (MLT) have recently been proposed for modelling convective heat transport inside stars. The ideal formulation is one that does not involve any free parameters. However, in our present state of ignorance we still need at least one free paramet...
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| Outros Autores: | , |
| Formato: | article |
| Idioma: | eng |
| Publicado em: |
1996
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| Texto completo: | https://hdl.handle.net/10216/64731 |
| País: | Portugal |
| Oai: | oai:repositorio-aberto.up.pt:10216/64731 |