Scaling law of the plasma turbulence with non conservative fluxes
arXiv:astro-ph/0509845 · doi:10.1103/PhysRevE.72.046407
Abstract
It is shown that in the presence of anisotropic kinetic dissipation existence of scale invariant power law spectrum of plasma turbulence is possible. Obtained scale invariant spectrum is not associated with the constant flux of any physical quantity. Application of the model to the high frequency part of the solar wind turbulence is discussed.
Phys Rev E, accepted