ИСТИНА

In this paper the high energy neutrino (1 TeV-100 PeV) spectrum was modelled from active galactic nuclei - possible sources of astrophysical neutrinos. The results are obtained in model where accretion disc emitted in UV-optical range located inside electron plasma cloud - hot corona. Using Monte-Carlo approach for photopion interactions it was shown that the resulting spectrum can explain the detected neutrino flux from IceCube.