PACS numbers

95.85.Ry Neutrino, muon, pion, and other elementary particles; cosmic rays
  1. S.V. Troitsky “Cosmic particles with energies above 1019 eV: a brief summary of resultsPhys. Usp. 56 304–310 (2013)
    95.55.Vj, 95.85.Ry, 98.70.Sa (all)
  2. G.A. Gusev, B.N. Lomonosov et alIce satellites of planets of the Solar System and the on-orbit radio detection of ultrahigh-energy particlesPhys. Usp. 53 915–921 (2010)
    95.55.Vj, 95.85.Ry, 96.50.S− (all)
  3. L.I. Dorman “Cosmic ray variations and space weatherPhys. Usp. 53 496–503 (2010)
    94.30.−d, 95.85.Ry, 96.50.S− (all)
  4. O.G. Ryazhskaya “Neutrinos from stellar core collapses: present status of experimentsPhys. Usp. 49 1017–1027 (2006)
    95.55.Vj, 95.85.Ry, 97.60.−s (all)
  5. V.A. Ryabov “Ultrahigh-energy neutrinos from astrophysical sources and superheavy particle decaysPhys. Usp. 49 905–936 (2006)
    12.60.−i, 13.15.+g, 95.55.Vj, 95.85.Ry, 96.50.S− (all)
  6. G.B. Khristiansen “Apparatus for studying extremely high energy cosmic raysSov. Phys. Usp. 30 539–541 (1987)
    98.70.Sa, 95.85.Ry (all)
  7. V.A. Tsarev “Geophysical applications of neutrino beamsSov. Phys. Usp. 28 940–940 (1985)
    95.85.Ry, 91.35.Lj, 91.30.Px (all)
  8. M.A. Gintzburg “Visual observation of cosmic raysSov. Phys. Usp. 16 163–164 (1973)
    96.50.sf, 95.85.Ry, 96.50.Vg, 96.60.Vg (all)
  9. D.V. Skobel’tsyn “The outstanding russian physicist S. I. VavilovSov. Phys. Usp. 4 737–739 (1962)
    98.70.Dk, 95.85.Ry, 95.85.Pw (all)
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