General Relativistic Magnetohydrodynamics Mean-Field Dynamos
Large-scale, ordered magnetic fields in several astrophysical sources are supposed to be originated, and maintained against dissipation, by the combined amplifying action of rotation and small-scale turbulence. For instance, in the solar interior, the so-called <inline-formula><math xmlns="http://ww...
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| Principais autores: | , , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
MDPI AG
2022-02-01
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| coleção: | Fluids |
| Assuntos: | |
| Acesso em linha: | https://www.mdpi.com/2311-5521/7/2/87 |
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