Abstract
The method of analysis and possibilities of identification of neutrino bursts from collapsing stars using a spatial distribution of pulses in the multimodular installations, like the Large Volume Detector at the Gran Sasso Laboratory, Liquid Scintillation Detector (Mont Blanc) and Baksan Scintillation Telescope, are discussed. The method could be applicable for any position sensitive detector. By the spatial distribution analysis the burst imitation probability can be decreased by at least 2 orders of magnitude, without significant loss of sensitivity, for currently predicted number of the neutrino interactions.
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