A more realistic representation of overshoot at the base of the solar convective envelope as seen by helioseismology
The stratification near the base of the Sun's convective envelope is governed by processes of convective overshooting and element diffusion, and the region is widely believed to play a key role in the solar dynamo. The stratification in that region gives rise to a characteristic signal in the f...
| Autor principal: | |
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| Outros Autores: | , , |
| Formato: | article |
| Idioma: | eng |
| Publicado em: |
2011
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| Assuntos: | |
| Texto completo: | https://repositorio-aberto.up.pt/handle/10216/98386 |
| País: | Portugal |
| Oai: | oai:repositorio-aberto.up.pt:10216/98386 |