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)Medline RefWorks RT Journal T1 Cherenkov detectors for high energy neutrino astrophysics A1 Dzhilkibaev,Ja.-A.M. A1 Domogatsky,G.V. A1 Suvorova,O.V. PB Physics-Uspekhi PY 2015 FD 10 May, 2015 JF Physics-Uspekhi JO Phys. Usp. VO 58 IS 5 SP 495-502 DO 10.3367/UFNe.0185.201505j.0531 LK https://ufn.ru/en/articles/2015/5/i/ 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