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A generalized model with three active and three sterile neutrinos isconsidered on the basis of the experimental data, which allow existence ofanomalies beyond the minimally extended Standard Model with three activeneutrinos with different masses. One of the sterile neutrinos is assumed to becomparatively heavy versus the two others, that is corresponding to the$(3+1+2)$-model of neutrino. The model parameters used for the description ofoscillations of both active and sterile massive neutrinos are given. In theapproximation of CP-conservation, the solar neutrino oscillationcharacteristics together with the sterile neutrino contributions have beenevaluated taking into account the neutrino interaction with the matter insidethe Sun. The results obtained are in accordance with the observational data andcan further be used for the description of neutrino oscillations inastrophysical and terrestrial environments and in search of sterile neutrinos.

Active and sterile neutrino oscillations inside the Sun in a phenomenological (3+1+2)-model