Fig. 6


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Background corona and solar wind solutions with the AWSoM-R model for solar minimum and maximum conditions. The background solar wind is driven by an outward going photospheric turbulent energy flux per unit magnetic field of 1 MJ m−2 s−1 Tesla−1 (CR2209) and by 0.45 MJ m−2 s−1 Tesla−1 (CR2123).

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