At the moment, it is known that when extrapolating, based on data obtained from probes, including Voyagers, the Sun generates radiation equivalent to 4 million tons of matter at the time of 4.5 billion. The magnitude of the solar constant equal to 1,360.8 W/m2 up to the atmosphere has been established for the years of the star’s existence [1—3; 10—11]. Based on the current model of star formation and the model of mass expenditure, the value is clearly formed that at the time of 5.6 billion years after the formation of the star, the radiation power will increase by 11% and amount to 1,532.47 W/m2, respectively [4; 6—7]. The resulting value may be sufficient to transform the model into a dynamic form.
For further modeling, we will take an equation capable of describing the phenomenon of radiation in the presence of radiation, with the condition that in this case no energy is supplied to the source from the outside or, in comparison with the values of solar radiation, the power of cosmic radiation can be ignored, which is demonstrated in practice. Despite the fact that even taking into account the presence of not a small number of sources of cosmic radiation, the percentage of radiation – the flux of charged particles, even compared with the solar neutrino and the flux of solar charged particles, is extremely small in percentage [5; 7—10]. Based on this, the main radiation energy is transmitted by photonic radiation.
In many works, the processes of radiation formation in the Sun and the process of energy transfer from the Sun to other planets, including to Earth, are considered, but the proposed technology for mathematical analysis of available data and the development of further radiation processes are not considered. Therefore, this study is relevant.
Materials and methods of research
To carry out the research, empirical materials that are well-known, relevant literature on the topic, as well as data obtained from international research papers were used [13—15; 18—19]. Numerous probes have been launched to measure the radiated energy, with the help of which radiation parameters are periodically studied. Within the framework of the ongoing research, methods of theoretical modelling, analysis, classification, the method of separation of variables (Fourier method), the method of using differential equations for modelling, with the resulting methods for determining their solutions, are applied.