Time-averaged wind fluxes vs. the plasma parameter β. The errorsare estimated through the standard deviation of the time -averaged sample. For stronger fields, the rates approximately follow the same power law as the dashed line, which is based on results of Béthune et al. (2017). For weaker fields, the photoevaporation begins to dominate, and the data points at β > 10⁷ indicate the influence of radiation shielding in the inner region, which results in lower mass fluxes overall.