Intermittency in MHD turbulence and coronal nanoflares modelling

High resolution numerical simulations, solar wind data analysis, and measurements at the edges of laboratory plasma devices have allowed for a huge progress in our understanding of MHD turbulence. The high resolution of solar wind measurements has allowed to characterize the intermittency observed a...

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Bibliographic Details
Main Authors: P. Veltri, G. Nigro, F. Malara, V. Carbone, A. Mangeney
Format: Article
Language:English
Published: Copernicus Publications 2005-01-01
Series:Nonlinear Processes in Geophysics
Online Access:http://www.nonlin-processes-geophys.net/12/245/2005/npg-12-245-2005.pdf