Finite dissipation and intermittency in magnetohydrodynamics

We present an analysis of data stemming from numerical simulations of decaying magnetohydrodynamic (MHD) turbulence up to grid resolution of 15363 points and up to Taylor Reynolds number of ∼1200. The initial conditions are such that the initial velocity and magnetic fields are helical and in equipa...

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Detalles Bibliográficos
Autores principales:	Mininni, P.D., Pouquet, A.
Formato:	JOUR
Materias:	Analysis of data Equipartition Fast reconnection Grid resolution Initial conditions Initial velocities Intermittency MHD flow Numerical simulation Solar environment Structure functions Taylor-Reynolds number Computer simulation languages Fluid dynamics Magnetohydrodynamics Reynolds number Solar wind Magnetic fields
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_15393755_v80_n2_p_Mininni
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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