Zobrazeno 1 - 10
of 55
pro vyhledávání: '"Pyatovsky S.E"'
Publikováno v:
In Astroparticle Physics November 2018 102:32-38
Akademický článek
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Autor:
Shaulov S.B., Beyl P.F., Beysembaev R.U., Beysembaeva E.A., Bezshapov S.P., Borisov A.S., Cherdyntceva K.V., Chernyavsky M.M., Chubenko A.P., Dalkarov O.D., Denisova V.G., Erlykin A.D., Kabanova N.V., Kanevskaya E.A., Kotelnikov K.A., Morozov A.E., Mukhamedshin R.A., Nam R.A., Nesterova N.M., Nikolskaya N.M., Pavluchenko V.P., Piskal V.V., Puchkov V.S., Pyatovsky S.E., Ryabov V.A., Sadykov T.Kh., Schepetov A.L., Smirnova M.D., Stepanov A.V., Uryson A.V., Vavilov Yu.N., Vildanov N.G., Vildanova L.I., Zayarnaya I.S., Zhanceitova J.K., Zhukov V.V.
Publikováno v:
EPJ Web of Conferences, Vol 145, p 17001 (2017)
The development of nuclear-electromagnetic cascade models in air in the late forties have shown informational content of the study of cores of extensive air showers (EAS). These investigations were the main goal in different experiments which were ca
Externí odkaz:
https://doaj.org/article/3dbfd66093284ad0ace093e2e791a0ba
Autor:
Borisov A.S., Denisova V.G., Guseva Z.M., Kanevskaya E.A., Pyatovsky S.E., Kogan M.G., Morozov A.E., Mukhamedshin R.A., Puchkov V.S., Shaulov S.B., Shoziyoev G.P., Smirnova M.D.
Publikováno v:
EPJ Web of Conferences, Vol 145, p 19008 (2017)
Characteristics of γ-ray families with halos (XREC, Pamir) and data of experiments with EAS are analyzed to estimate the proton and helium (p+He) fractions in the primary cosmic radiation at E0 = 1–100 PeV. It is shown that at energies E0 ∼ 1–
Externí odkaz:
https://doaj.org/article/25bb93c402d84b43889a50800f631ca8
Autor:
Borisov, A.S., Denisova, V.G., Guseva, Z.M., Kempa, J., Kanevskaya, E.A., Maximenko, V.M., Puchkov, V.S., Pyatovsky, S.E., Slavatinsky, S.A.
Publikováno v:
In Nuclear Physics B (Proceedings Supplements) 2008 175:143-148
Akademický článek
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Autor:
Amurina, I.A., Antonova, V.P., Autova, G.M., Babaev, M.K., Baygubekov, A.S., Beyl', P.A., Beisembaev, R.U., Bodunov-Skvortsov, A.E., Borisov, A.S., Cherdyntseva, K.V., Chubenko, A.P., Chubenko, P.A., Denisova, V.G., Drobzhev, V.I., Gudkova, E.N., Gurevich, A.V., Guseva, Z.M., Kanevskaya, E.A., Kempa, J., Kogan, M.G., Kostin, E.V., Kryakunova, O.N., Kruglov, A.V., Kryukov, S.V., Krylowa, M.I., Kupchishin, A.I., Managadze, A.K., Mart'yanov, I.S., Maximenko, V.M., Mukashev, K.M., Mukhamedeshin, R.A., Nam, R.A., Nesterova, N.M., Nuritdinov, Kh., Oskomov, V.V., Pavlyuchenko, V.P., Piscal', V.V., Polyakov, R.Yu., Puchkov, V.S., Pyatovsky, S.E., Rakobol'skaya, I.V., Roganova, T.M., Roinishvili, N.N., Ryabov, V.A., Saduev, N.O., Sadykov, T.Kh., Shaulov, S.B., Shchepetov, A.L., Slavatinsky, S.A., Stepanov, A.V., Sveshnikova, L.G., Shoiynbaeva, G.T., Tolegen, Zh.T., Vavilov, Yu.N., Vargasov, A.V., Vil'danov, N.G., Vil'danova, L.I., Yakovlev, V.I., Yuldashbaev, T.S., Zastrozhnova, N.N., Zatsepin, G.T., Zhukov, V.V.
Publikováno v:
In Nuclear Physics B (Proceedings Supplements) 2006 151(1):422-425
Autor:
Puchkov, V.S., Borisov, A.S., Guseva, Z.M., Denisova, V.G., Kanevskaya, E.A., Maximenko, V.M., Pyatovsky, S.E., Slavatinsky, S.A.
Publikováno v:
In Nuclear Physics B (Proceedings Supplements) 2006 151(1):236-239
Autor:
Borisov A.S., Chubenko A.P., Denisova V.G., Galkin V.I., Guseva Z.M., Kanevskaya E.A., Kogan M.G., Kulikov V.N., Morozov A.E., Mukhamedshin R.A., Puchkov V.S., Nazarov S.I., Pyatovsky S.E., Shoziyoev G.P., Smirnova M.D., Vargasov A.V.
Publikováno v:
EPJ Web of Conferences, Vol 99, p 10004 (2015)
The origin of the cosmic ray hadron excess observed in a deep uniform lead X-ray emulsion chamber (XREC) at depths larger than 70 radiation lengths is analyzed. We present preliminary experimental data on the absorption of cosmic ray hadrons in the t
Externí odkaz:
https://doaj.org/article/5c0815958f0d45a2898522df9f9dda24
Autor:
Pyatovsky S.E, Puchkov V.S., Mukhamedshin R.A., Morozov A.E., Maximenko V.M., Kogan M.G, Kanevskaya E.A., Denisova V.G., Guseva Z.M., Borisov A.S., Smirnova M.D.
Publikováno v:
EPJ Web of Conferences, Vol 52, p 04007 (2013)
Recently essential efforts were made to improve measurement routine with X-ray films exposed in the X-ray emulsion chambers at the Pamirs. Analysis of X-ray emulsion response upon recorded events show that γ-family energy and intensity in early publ
Externí odkaz:
https://doaj.org/article/d3615c077c384355837c40c3722962d8