Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: An application to the intracluster medium

The amplification of magnetic fields (MFs) in the intracluster medium (ICM) is attributed to turbulent dynamo (TD) action, which is generally derived in the collisional-MHD framework. However, this assumption is poorly justified a priori, since in the ICM the ion mean free path between collisions is...

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Detalles Bibliográficos
Autor principal:	Nakwacki, Maria Soledad
Publicado:	2014
Materias:	galaxies: clusters: intracluster medium magnetic fields magnetohydrodynamics (MHD) turbulence
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v781_n2_p_SantosLima http://hdl.handle.net/20.500.12110/paper_0004637X_v781_n2_p_SantosLima
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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