Meridional circulation dynamics in a cyclic convective dynamo
Surface observations indicate that the speed of the solar meridional circulation in the photosphere varies in anti-phase with the solar cycle. The current explanation for the source of this variation is that inflows into active regions alter the global surface pattern of the meridional circulation....
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| Outros Autores: | , , |
| Formato: | article |
| Idioma: | eng |
| Publicado em: |
2019
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| Assuntos: | |
| Texto completo: | http://hdl.handle.net/10400.1/12924 |
| País: | Portugal |
| Oai: | oai:sapientia.ualg.pt:10400.1/12924 |