CREATING A MODEL OF THE FALL OF SOLAR ENERGY IN CERTAIN COORDINATES

In the course of this study, a mathematical model of solar activity was created at the specified coordinates for a certain time, with the development of an appropriate algorithm of action. In the course of the study, a function was created with respect to a spherical coordinate system based on an approximate model of the planet and its irradiation system. Subsequently, empirically obtained boundary conditions were set for the function, so that a certain general form was turned into a particular form in the class of linear functions.