MAGNETIC FIELD AMPLIFICATION AND EVOLUTION IN TURBULENT COLLISIONLESS MAGNETOHYDRODYNAMICS: AN APPLICATION TO THE INTRACLUSTER MEDIUM

2013/05/24 by R. Santos-Lima, E. M. de Gouveia Dal Pino, G. Kowal +3 · 2 citations
Physics and Astronomy · #Anisotropy #Astrophysical plasma #Dynamo #Ionosphere and magnetosphere dynamics #Magnetic confinement fusion research #Magnetic field #Magnetohydrodynamics #Plasma #Relaxation (psychology) #Solar and Space Plasma Dynamics #Turbulence #astro-ph.CO #astro-ph.GA #astro-ph.HE #physics.plasm-ph

paper · pdf · doi:10.1088/0004-637x/781/2/84

24 pages, 12 figures, submitted to ApJ

arxiv created 2013/05/24 · openalex publication_date 2014/01/13 · arxiv updated 2015/06/16 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06

Abstract

MAGNETIC FIELD AMPLIFICATION AND EVOLUTION IN TURBULENT COLLISIONLESS MAGNETOHYDRODYNAMICS: AN APPLICATION TO THE INTRACLUSTER MEDIUM, R. Santos-Lima, E. M. de Gouveia Dal Pino, G. Kowal, D. Falceta-Gonçalves, A. Lazarian, M. S. Nakwacki

Citations

• The Boltzmann equation an d the one-fluid hydromagnetic equations in the absence of particle collisions
• Compressible turbulence in galaxy clusters: physics and stochastic particle re-acceleration
• A non-linear theory of the parallel firehose and gyrothermal instabilities in a weakly collisional plasma
• Magnetic Field in Clusters of Galaxies

Cited by

• Turbulent dynamo in the terrestrial magnetosheath
• Suppressed heat conductivity in the intracluster medium: implications for the magneto-thermal instability