  Opportunity of the solar flares (SF's) prediction observing the solar
neutrino fluxes is investigated. In three neutrino generations the evolution of
the neutrino flux traveling the coupled sunspots (CS's) which are the SF source
is considered. It is assumed that the neutrinos possess both the dipole
magnetic moment and the anapole moment while the magnetic field above the CS's
may reach the values $10^5-10^6$ Gs, displays the twisting nature and has the
nonpotential character. The possible resonance conversions of the solar
neutrino flux are examined. Since the $\nu_{eL}\to \nu_{\mu L}$ resonance takes
place before the convective zone, its existence can in no way be connected with
the SF. However, when the solar neutrino flux moves through the CS's in the
preflare period, then it may undergo the additional resonance conversions and,
as a result, depleting the electron neutrinos flux may be observed.
