The model of coronal hole with microwave observational data taking into account the solar wind flows

The renew non-hydrostatic model of electron density, temperature and velocity distribution with height in coronal hole (CH) is build. The presented model is based on the measurements of magnetic field in CH with RATAN-600 observations and on the assumption about equality of magnetic and kinetic energy of upward plasma flows in CH at heights of generation of radio emission in wavelength range 20 – 30 cm. To construct this model the observational spectrum of brightness temperatures of CH in wavelength range 2 – 30 cm is used. The first results of modeling are presented.