Turbulence in the Solar Wind by Roberto Bruno & Vincenzo Carbone

Author:Roberto Bruno & Vincenzo Carbone
Language: eng
Format: epub
Publisher: Springer International Publishing, Cham

(4.18)

where are the Elsässer variables, V A is the Alfvén velocity, ρ is the plasma density, I is the identity matrix, NL ± are nonlinear dissipation terms and S ± are source terms. NL ± and S ± are modeled separately for outward and inward modes. The model is then based on the following seven coupled turbulence transport equations, one for each of the parameters listed above plus one that describes the transport equation for the solar wind temperature in the super-Alfvénic solar wind.

(4.19)

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