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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...

Täydet tiedot

Tallennettuna:
Bibliografiset tiedot
Päätekijät: Luca Del Zanna , Niccolò Tomei, Kevin Franceschetti, Matteo Bugli, Niccolò Bucciantini
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: MDPI AG 2022-02-01
Sarja:Fluids
Aiheet:
Linkit:https://www.mdpi.com/2311-5521/7/2/87
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