We present the results of determining the integral flux of protons and alpha particles, which make up the bulk of the mass carried away from the Sun. The flow parameters were taken from the observation archive of the Ulysses spacecraft. We used a self-written program to process observations. 2-dimensional and 3-dimensional graphs are plotted that clearly illustrate the processes occurring in the solar wind. The result obtained in this way is in good agreement with the results presented by other authors obtained using other methods.