On the formation of the corona and solar wind fast fluxes over coronal holes

Consideration is being given to the corona formation and solar wind flow over coronal holes in the model with the energy source in the form of magnetohydrodynamic waves. The magnetic field structure is suggested to be quasimonopole. It is shown that superradial divergence of magnetic force lines results to stronger, as compared to radial field, effect of flow on thermal conditions of the corona. This suggests lower temperature and plasma density values in the corona, as compared to background ones, and higher flow rates