A global 3D MHD model with wave-turbulence heating reproduces the essential observed charge states of solar wind ions for two Carrington rotations.
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Ion Charge States from a Global Time-Dependent Wave-Turbulence-Driven Model of the Solar Wind: Comparison with in-situ Measurements
A global 3D MHD model with wave-turbulence heating reproduces the essential observed charge states of solar wind ions for two Carrington rotations.