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The inertial-range spectrum of fully developed magnetohydrodynamic turbulence

This note suggests that the classical inertial-range spectrum of fully developed Magnetohydrodynamic (MHD) turbulence should be modified in presence of intermittency. We show that the pseudo-energy density spectra of both the Alfvenic modes follow a k −(3/2+Ψ) power law and, introducing two intermittency cascade models, we find the function Ψ