Khokhlov, S. S.S. S.KhokhlovAmelchakov, M. B.M. B.AmelchakovBarbashina, N. S.N. S.BarbashinaBogdanov, A. G.A. G.BogdanovBurtsev, V. D.V. D.BurtsevChernov, D. V.D. V.ChernovDmitrieva, A. N.A. N.DmitrievaDushkin, L. I.L. I.DushkinKhomyakov, V. A.V. A.KhomyakovKindin, V. V.V. V.KindinKokoulin, R. P.R. P.KokoulinKompaniets, K. G.K. G.KompanietsKovylyaeva, E. A.E. A.KovylyaevaKruglikova, V. S.V. S.KruglikovaMannocchi, G.G.MannocchiOvchinnikov, V. V.V. V.OvchinnikovPetrukhin, A. A.A. A.PetrukhinSaavedra, O.O.SaavedraShulzhenko, I. A.I. A.ShulzhenkoShutenko, V. V.V. V.ShutenkoTRINCHERO, GIAN CARLOGIAN CARLOTRINCHEROYashin, I. I.I. I.YashinZadeba, E. A.E. A.Zadeba2020-06-032020-06-0320151742-6588http://hdl.handle.net/20.500.12386/25887A technique for the reconstruction of cascade profiles by means of Cherenkov radiation in the water of the NEVOD detector is discussed. NEVOD is equipped with a dense spatial lattice of optical modules. The analyzed cascades have been generated either along near-horizontal muons (zenith angles between 85 and 90°), which's tracks are reconstructed by means of the tracking detector DECOR, or by muons with unknown tracks over a wider zenith angle range of 50-90°. Mean cascade profiles and energy spectra of cascades measured during the experimental series of about 7950 hours of ‘live time’ are presented. <P />STAMPAenConference paper10.1088/1742-6596/632/1/0120382-s2.0-84940706258000362286200038https://iopscience.iop.org/article/10.1088/1742-6596/632/1/0120382015JPhCS.632a2038KFIS/05 - ASTRONOMIA E ASTROFISICA