Detection of Solar Flare Neutrinos

An attempt is made to estimate possible neutrino fluxes on the basis of observations of solar flares from the opposite side of the sun. In the case where such flares generate a number of protons of the order of 10 to the 34th, approximately 200 neutrino events can be registered by a detector whose mass is of the order of one million tons. Such solar flares occur several times/solar cycle.