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1. Workshop тАЬCosmic Ray Physics Large Scale Experiments at the Second Decade of
... The Council on Complex Problems of Cosmic Rays of the Russian Academy of Sciences and the Skobeltsyn Institute of Nuclear Physics (SINP) of Lomonosov Moscow State University are planning to held a workshop "Cosmic Ray Physics Large Scale Experiments at the Second Decade of the 21st Century" on May 16-18 2011 at the Moscow State University. ... The Workshop banquet will be held on Tuesday, May 17 th . ... Workshop тАЬCosmic Ray Physics Large Scale Experiments at the Second Decade of the 21st Century"...
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Ссылки http://tunka.sinp.msu.ru/en/ -- 22.2 Кб -- 04.02.2013
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2. http://tunka.sinp.msu.ru/en/presentation/Ptuskin.pdf
... Bohm limit DB=vrg/3: Emax Emax ush 0.3 Ze B Rsh c 1014(B/Bism) Z eV B Hillas criterion ! ... Voelk 2000; Kang Jones 2006) - Bohm diffusion in amplified magnetic field B2/8 = 0.035 u2/2 ( Voelk et al. 2005 empirical; Bell 2004 , Zirakashvili VP 2008 theoretical) - account for Alfvenic drift w = u + Va upstream and downstream - relative SNR rates: SN Ia : IIP : Ib/c : IIb = 0.32 : 0.44 : 0.22 : 0.02 Chevalier 2004 , Leaman 2008, Smart et al 2004, Berezinsky et al 2006 Das et al. ...
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Ссылки http://tunka.sinp.msu.ru/en/presentation/Ptuskin.pdf -- 1402.1 Кб -- 22.05.2011
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3. http://tunka.sinp.msu.ru/en/presentation/Dedenko.pdf
Fluctuation in EAS development and estimates of energy and composition of the primary radiation by L. Dedenko, SINP, MSU 1) surface scintillation detectors (SD) 2) detectors of the Vavilov-Cherenkov radiation (VCR) 3) underground detectors of muons (UD) (with the threshold energy ~1 GeV). Yakutsk array Detectors readings Ї The various particles Ї of Extensive Air Showers (EAS) Ї at the observation level Ї hit detectors Ї and induce some signals sampled as Ї detector readings 18.05.2011. IWS. ...
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Ссылки http://tunka.sinp.msu.ru/en/presentation/Dedenko.pdf -- 2599.4 Кб -- 22.05.2011
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4. http://tunka.sinp.msu.ru/en/presentation/Khrenov.pdf
TUS/KLYPVE Program for Observation of Extreme Energy Cosmic Rays from Space B.A. Khrenov DV Skobeltsyn Institute of Nuclear Physics of MV Lomonosov Moscow State University Workshop "Cosmic Ray Large Scale Experiments in the Second Decade of the 21st Century" 17 May 2011 TUS/KLYPVE collaboration SINP MSU, JINR (Dubna), RSC "Energia", Consortium "Space Regatta" EWHA University (Seoul, Korea) Puebla University (Mexico) Universities of Japan, RIKEN (Tokyo). ... Digital oscilloscopes for UV flashes. ...
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Ссылки http://tunka.sinp.msu.ru/en/presentation/Khrenov.pdf -- 1688.1 Кб -- 22.05.2011
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5. http://tunka.sinp.msu.ru/en/presentation/Shpiering.pdf
... A p P EC Astropar ticle Physics for Europe Ї Cosmic rays: A large array for the detection of charged cosmic rays ( Auger North) Ї Gamma rays: A large array of Cherenkov Telescopes for detection of cosmic high energy gamma-rays ( CTA ) Ї High energy neutrinos: A cubic kilometre-scale neutrino telescope in the Mediterranean (KM3NeT) Ї Dark matter search: Ton-scale detectors ... A p P EC Astropar ticle Physics for Europe Ї Cosmic rays: ґ ґ ґ ґ ґ AMS detector launched. ...
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Ссылки http://tunka.sinp.msu.ru/en/presentation/Shpiering.pdf -- 2300.6 Кб -- 22.05.2011
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6. http://tunka.sinp.msu.ru/en/presentation/Zirakashvili.pdf
Gamma-quanta from SNRs V.N.Zirakashvili Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Russian Academy of Sciences (IZMIRAN), 142190 Troitsk, Moscow Region, Russia Outline Ї Acceleration of particles at forward and reverse shocks in SNRs Ї Amplification of magnetic fields Ї Modeling of broad-band emission Ї Radioactivity and electron acceleration Diffusive Shock ... 2010) . ... Cosmic ray positrons can be accelerated at reverse shocks of SNRs. ...
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Ссылки http://tunka.sinp.msu.ru/en/presentation/Zirakashvili.pdf -- 2158.2 Кб -- 22.05.2011
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7. http://tunka.sinp.msu.ru/en/presentation/Sveshnikova.pdf
... 5) Two variant of calculation: Main 1 (absence of SNRs in the Earth vicinity with Emax =4 PeV ) and Main 2 (where 4 SNRs accelerate to 4 PeV ) give more or less similar structures around the knee Here we need to know MetaGalactic Sum Gal+Metag 025 0.20 Ї 10 7 Ї F(E) E 10 6 P He 3 .0 Fe Ї 10 5 C,O Si Pure Galactic Ї 10 4 10 4 10 5 10 6 10 7 10 8 10 9 10 10 10 11 10 12 E, GeV Contribution of nearby actual sources 10 1 Main 2 all p he cno si fe nearby ...
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Ссылки http://tunka.sinp.msu.ru/en/presentation/Sveshnikova.pdf -- 665.7 Кб -- 22.05.2011
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8. http://tunka.sinp.msu.ru/en/presentation/horns_vhe.pdf
Gamma-rays above 10 TeV Dieter Horns ґ University Hamburg RXJ1713-3946 [HESS Coll. ... The indirect path to the accelerator sky Dieter Horns ґ University Hamburg Is it a good deal? [astro-ph/0607109] Unveiling Cosmic Ray accelerators: Interstellar medium ( B-field + gas + photons) Accelerated Nuclei Meson production via inelastic scattering Gamma-rays , Neutrinos Cosmic rays Neutral particles (photons neutrinos) retain directional information: Accelerator sky Charged particles ( ...
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Ссылки http://tunka.sinp.msu.ru/en/presentation/horns_vhe.pdf -- 2821.8 Кб -- 22.05.2011
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