Mirahmadaga BM
Compton and inverse Compton effect in solar wind plasma, equations obtained on the basis of magnetohydrodynamic theory for one-particle plasma were investigated. The radial dependences of the solar wind speed were obtained and analyzed using MHD equations. The results are important in explaining the acceleration mechanism of cosmic plasma particles, in studying the evolution process of the Sun and stars, as well as in the study of the factors affecting the operation of radio electronic control devices.