Yılmaz, AliLori, MaurizioDenizli, HalukOyulmaz, Kaan YükselAtik, Şeyma YılmazKeskin, Umut2021-06-232021-06-2320171824-8039https://hdl.handle.net/20.500.12491/3950https://www.scopus.com/inward/record.uri?eid=2-s2.0-85046053593&partnerID=40&md5=b596526296008a2ad98e872dfc98f5f435th International Cosmic Ray Conference, ICRC 2017 -- 10 July 2017 through 20 July 2017 -- -- 135186In the neutrino physics the direct measurement of the cosmogenic neutrino at energy of 1015 -1018 eV is still a challenging item. The most recent analysis of IceCube data results in an energy spectrum between 1013 and 1016 eV. We present the preliminary results of detailed Monte Carlo simulation of tau-induced air shower. In this study we consider the highest tau decay branching ratio (?- ?0) at different energies (1016 - 1018 eV) generated by CORSIKA to evaluate the detection efficiency of the TAU-shoWER (TAUWER) array. It is designed as a future experiment for Ultra High Energetic tau-neutrino (UHE v?) astronomy to use Earth neutrino skimming strategy. The parameters (the distance from array plane to the emerging point and the neutrino energy) to optimize the detection efficiency and the trigger design for the TAUWER array setup are presented. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0).eninfo:eu-repo/semantics/closedAccessAtomic PhysicsCosmic RaysCosmologyIntelligent SystemsConference Object2-s2.0-85046053593N/A