ИСТИНА

Purpose of this paper - to calculate the theoretical neutrino flux based on the evolutionary solar model constructed with a view of gelioseysmic data. We simulate the spectrum of neutrinos emitted in the reactions of p-p and CNO cycles, taking into account possible deviations from the equilibrium concentrations of the intermediate components. The proportion of muon and electron neutrinos in the flux are calculated, taking into account the oscillations in the plasma, under certain assumptions about the neutrino parameters. The simulation results are compared with the observed solar neutrinos flux.