Three dimensional simulations of Hall magnetohydrodynamics

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Turbulent flows take place in a large variety of astrophysical objects, and often times are the source of dynamo generated magnetic fields. Much of the progress in our understanding of dynamo mechanisms, has been made within the theoretical framework of magnetohydrodynamics (MHD). However, for suffi...

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Detalles Bibliográficos
Autor principal: Gómez, D.O.
Formato: Artículo publishedVersion
Publicado: 2010
Materias:
ISM: magnetic fields
MHD
turbulence
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS274_p433_Gomez
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_17439213_v6_nS274_p433_Gomez_oai
Aporte de:
Repositorio Digital de la Universidad de Buenos Aires (UBA) de Universidad de Buenos Aires

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