This review discusses the current status of and prospects for large-scale Cherenkov detectors that operate in deep-underwater- and under-ice environments (Lake Baikal, Mediterranean sea, Antarctica) and which have, in the last decades, become the primary tool for measuring high energy neutrino fluxes.
110th anniversary of the birth of P.A. Cherenkov (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 17 December 2014)

Keywords: Cherenkov radiation, neutrino telescopes, neutrino astrophysics PACS: 29.40.Ka, 41.60.Bq, 95.55.Vj (all) DOI: 10.3367/UFNe.0185.201505j.0531 URL: https://ufn.ru/en/articles/2015/5/i/ 000360073200009 2-s2.0-84938834012 2015PhyU...58..495D Citation: Dzhilkibaev Ja-A M, Domogatsky G V, Suvorova O V "Cherenkov detectors for high energy neutrino astrophysics" Phys. Usp. 58 495–502 (2015) BibTexBibNote ® (generic)BibNote ® (RIS)MedlineRefWorks Received: 16th, March 2015, accepted: 17th, December 2014 Оригинал: Джилкибаев Ж-А М, Домогацкий Г В, Суворова О В «Черенковские детекторы в нейтринной астрофизике высоких энергий» УФН 185 531–539 (2015); DOI: 10.3367/UFNr.0185.201505j.0531 P.A. Cerenkov is author of Physics-Uspekhi