Abstract:We investigated plasma turbulence in the context of solar wind. We concentrated
on properties of ideal second-order magneto-hydrodynamic (MHD) and Hall MHD invariants. We studied the results of a two-dimensional hybrid simulation of decaying plasma turbulence
with an initial large cross helicity and a negligible magnetic helicity.
We investigated the evolution of the combined energy and the cross, kinetic, mixed,
and magnetic helicities. For the combined (kinetic plus magnetic) energy and the
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