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The largest Solar flare have been recorded in gamma flash and hard spectra upto tens GeV energy. The present building and upgrade of Hyper-Kamiokande (HK)and IceCube (as well as Deep Core, PINGU) neutrino detectors do offer a novelway to largest trace of solar Flare: their sudden anti-neutrino (or neutrino)flare made by proton scattering and pion decays via Delta resonance production.These signals might be observable at largest flare by HK via soft spectra up totens- hundred MeV energy and by IceCube-PINGU at higher, GeV up to hundred GeV,energies. We show the expected rate of signals for the most powerful solarflare occurred in recent decades.

Observing future Solar Flare Neutrino in Hyper-KamioKande in Japan, Korea and in IceCube