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Neutrino air showers can be formed in any part of the atmosphere passing along was in the matter due to its physical properties. In general, air showersproduced by neutrinos are highly inclined and formed near the ground level,i.e. young showers. Therefore, one should expect a large number of peaks in thesignal of such air showers [1, 2, 3].  The goal of our work is to search for air shower candidates produced byneutrino. For this purposes, we analyzed large amount of data fromscintillation detectors with different area and energy thresholds [1, 2].  Preliminary analysis of Yakutsk array data indicated the absence of airshower produced by neutrino, but it does not mean that such air showers doesnot exist. It is going to need a further analysis of highly inclined showers.In order to do that improved methodology for recording and processing of airshowers required.

Search for Neutrino Generated Air Shower Candidates with Energy More than 5$\cdot$10$^{18}$ eV and Zenith Angle $\theta$ $\geq$ 50$^\circ$