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Since the end of the eighties and in response to a reported increase in thetotal neutrino flux in the Homestake experiment in coincidence with solarflares, solar neutrino detectors have searched for solar flare signals. Eventhough these detectors have used different solar flare samples and analyses,none of them has been able to confirm the possible signal seen by Homestake.Neutrinos from the decay of mesons, which are themselves produced in collisionsof accelerated ions with the solar atmosphere would provide a novel window onthe underlying physics of the hadronic acceleration and interaction processesduring solar flares. Solar flare neutrino flux measurements would indeed helpto constrain current parameters such as the composition of the acceleratedflux, the proton/ion spectral index and the high energy cutoff or the magneticconfiguration in the interaction region. We describe here a new way to searchfor these neutrinos by considering a specific solar flare sample and a datadriven time window template which will improve the likelihood of neutrinodetection.

On the detection of neutrinos from solar flares using pion-decay photons to provide a time window template