Ìóõàìåäøèí Ðàóô Àäãàìîâè÷Í364,7289,524.01.2020
Ìóõàìåäøèí Ðàóô Àäãàìîâè÷, 3.12.1948, ä.ô.-ì.í.,
Âåäóùèé íàó÷íûé ñîòðóäíèê, è.î. çàâ. Ëàáîðàòîðèè íåéòðèííîé àñòðîôèçèêè, ÎËÂÝÍÀ

1) Èíäèâèäóàëüíûé ÏÐÍÄ                  = 364.73
2) ÏÐÍÄ ðóêîâîäèòåëÿ    = 0.50*364.7+ 0.75*137.6   = 289.48

Ñòàòüè â çàðóáåæíûõ æóðíàëàõ
1.   S.B. Shaulov, P.F. Beyl, R.U. Beysembaev, E.A. Beysembaeva, S.P. Bezshapov, A.S. Borisov, K.V. Cherdyntceva, M.M. Chernyavsky, A.P. Chubenko, O.D. Dalkarov, V.G. Denisova, A.D. Erlykin, N.V. Kabanova, E.A. Kanevskaya, K.A. Kotelnikov, A.E. Morozov, R.A. Mukhamedshin, R.A. Nam, N.M. Nesterova, N.M. Nikolskaya, V.P. Pavluchenko, V.V. Piskal, V.S. Puchkov, S.E. Pyatovsky, V.A. Ryabov, T.Kh. Sadykov, A.L. Schepetov, M.D. Smirnova, A.V. Stepanov, A.V. Uryson, Yu.N. Vavilov, N.G. Vildanov, L.I. Vildanova, I.S. Zayarnaya, J.K. Zhanceitova and V.V. Zhukov. Investigation of EAS cores. EPJ Web of Conferences 145 (2017) 17001                          ÏÐÍÄ = 1.20 (= 8*1.5*0.1)
2.   R.A. Mukhamedshin. Does superhigh-energy cosmic-ray coplanarity contradict LHC data? European Physical Journal C (2019) 79: 441. https://doi.org/10.1140/epjc/s10052-019-6931-0                            ÏÐÍÄ = 145.29 (=4.843*30)
3.   R.A. Mukhamedshin. FANSY 2.0: A Monte Carlo tool for study of superhigh-energy cosmic-ray interactions. Proton-proton interactions. Eur. Phys. J. Plus (2019) 134: 584. https://doi.org/10.1140/epjp/i2019-12933-2          ÏÐÍÄ = 78.36 (=2.612*30)
4.   R.A. Mukhamedshin, V. S. Puchkov, S. E. Pyatovsky, and S. B. Shaulov. Gamma-ray families with halos observed by X-ray emulsion chamber in EAS and the estimate of the p+He fraction in primary cosmic rays at E0 = 1 – 100 PeV. Bulletin of the Lebedev Physics Institute (2018), Vol. 45, No. 1, pp. 380-384.            ÏÐÍÄ = 6.93 (=0.308*1.5*60/4)         
5.   R.A.Mukhamedshin, V.S.Puchkov, S.E.Pyatovsky, S.B.Shaulov. Analysis of gamma-ray families with halos and estimation of mass composition of primary cosmic radiation at energies 1 –100 PeV. Astroparticle Physics 102 (2018) 32–38. DOI: 10.1016/j.astropartphys.2018.05.005
                           ÏÐÍÄ = 62.15 (=5.524*1.5*30/4)
6.   K.M. Mukashev, A.Kh. Arginova, A.D. Baisenova, B.A. Iskakov, R.A. Mukhamedshin, O.A. Novolodskaya, V.V. Piskal, V.A. Ryabov, T.Kh. Sadykov, A.S. Serikkanov, Y.M. Tautaev, V.V. Zhukov, N.N. Zastrozhnova. Search for structures in the distribution of particles from the central area of wide atmospheric showers conducted on the Adron-55 installation. Physical Sciences and Technology, v. 6, n. 1, p. 75-83 (2019).       ÏÐÍÄ = 1.20 (= 8*1.5*0.1)
7.   R Mukhamedshin1 and T Sadykov. Do LHC data contradict superhigh-energy cosmic-ray coplanarity of most energetic particles? 2019 J. Phys.: Conf. Ser. 1181 012089
                           ÏÐÍÄ = 6.00 (= 8*1.5/2)
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Èòîãî:                         ÏÐÍÄ = 301.13

Ñòàòüè â ðîññèéñêèõ æóðíàëàõ
1.   Ð.À. Ìóõàìåäøèí, Ñ.Å.Ïÿòîâñêèé, Â.Ñ. Ïó÷êîâ, Ñ.Á.Øàóëîâ. ?-ñåìåéñòâà ñ «ãàëî» ïðè íàáëþäåíèè ØÀË â ÐÝÊ è îöåíêà äîëè p+He â ÏÊË ïðè Å0=1 – 100 ÏýÂ. Êðàòêèå ñîîáùåíèÿ ïî ôèçèêå ÔÈÀÍ, ¹ 12 (2017) 64-72       ÏÐÍÄ = 9.40 (= 0.414*1.5*60/4)
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Èòîãî:                         ÏÐÍÄ = 9.40

Ïðåïðèíòû ýëåêòðîííûå:
1.   A.P.Chubenko, A.L.Shepetov, V.P.Antonova, R.U.Beisembayev, A.S.Borisov, O.D. Dalkarov, O.N.Kryakunova, K.M.Mukashev, R.A.Mukhamedshin, R.A.Nam, N.F.Nikolaevsky, V.P.Pavlyuchenko, V.V.Piscal, V.S.Puchkov, V.A.Ryabov, T.Kh.Sadykov, N.O.Saduev, N.M.Salikhov, S.B.Shaulov, A.V.Stepanov, N.G. Vildanov, L.I.Vildanova, M.I.Vildanova, N.N.Zastrozhnova, V.V.Zhukov. New complex EAS installation of the Tien Shan mountain cosmic ray station. arXiv:1912.13356v1 [astro-ph.HE]       ÏÐÍÄ = 0.45 (=3*1.5*0.1)
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Èòîãî:                         ÏÐÍÄ = 0.45

Äîêëàäû íà êîíôåðåíöèÿõ
1.   A.S. Borisov, V.G. Denisova, V.I. Galkin, Z.M. Guseva, E.A. Kanevskaya, M.G. Kogan, R.A. Mukhamedshin, S.I. Nazarov, V.S. Puchkov, S.E.Pyatovsky, M.D. Smirnova, A.V. Vargasov. Investigation of abnormal absorption of cosmic-ray hadrons in lead calorimeters. ISVHECRI 2018 (Nagoya), May 21–25, 2018 (oral)        https://indico.cern.ch/event/639198/timetable/ #20180521.detailed/                   ÏÐÍÄ = 3.75 (=1.5*15.0*0.1)
2.   R.A. Mukhamedshin. Does superhigh-energy cosmic-ray coplanarity contradict LHC data. E+CRS 2018 (Barnaul) July 5-10, 2018 (oral)   https://ecrs18.asu.ru/event/1/program                               ÏÐÍÄ = 25.00
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Èòîãî:                         ÏÐÍÄ = 28.75

Ìåæäóíàðîäíàÿ øêîëà
1.   Ìóõàìåäøèí Ð.À. Ââåäåíèå â ìîäåëèðîâàíèå âçàèìîäåéñòâèé ýëåìåíòàðíûõ ÷àñòèö ñ âåùåñòâîì ìåòîäîì Ìîíòå-Êàðëî. 5-ÿ Ìåæäóíàðîäíàÿ øêîëà ìîëîäûõ ó÷åíûõ ÑÍà «Ñìåæíûå ïðîáëåìû ôèçèêè è àñòðîôèçèêè ÷àñòèö ñâåðõâûñîêèõ ýíåðãèé», 26.08 – 01.09 2018 ã., ã. Àëìàòû (ÐÊ)    http://school-2018.tien-shan.org/   ÏÐÍÄ = 25.0
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Èòîãî:                         ÏÐÍÄ = 25.0

ÂÑÅÃÎ:                         ÏÐÍÄ = 364.73