Scaling law of plasma turbulence with nonconservative fluxes.
It is shown that in the presence of anisotropic kinetic dissipation existence of the scale invariant power law spectrum of plasma turbulence is possible. The 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.
Gogoberidze
Grigol
G
Georgian National Astrophysical Observatory, 2a Kazbegi Ave., 0160 Tbilisi, Georgia. gogober@geo.net.ge