PACS numbers

95.55.Vj Neutrino, muon, pion, and other elementary particle detectors; cosmic ray detectors 96.50.sb Composition, energy spectra and interactions 96.50.sh Interplanetary propagation and effects
  1. A.D. Filonenko “Radio emission of extensive air showers58 633–669 (2015)
    95.55.Vj, 98.70.Sa (all)
  2. A.A. Petrukhin “Cherenkov water detector NEVOD58 486–494 (2015)
    29.40.Ka, 95.55.Vj, 96.50.S− (all)
  3. Ja.-A.M. Dzhilkibaev, G.V. Domogatsky, O.V. Suvorova “Cherenkov detectors for high energy neutrino astrophysics58 495–502 (2015)
    29.40.Ka, 41.60.Bq, 95.55.Vj (all)
  4. Ch. Spiering “High-energy neutrino astronomy: a glimpse of the Promised Land57 470–481 (2014)
    13.15.+g, 95.55.Vj, 98.70.Vc (all)
  5. A.V. Derbin “Solar neutrino experiments57 512–524 (2014)
    26.65.+t, 14.60.Pq, 95.55.Vj (all)
  6. S.V. Troitsky “Cosmic particles with energies above 1019 eV: a brief summary of results56 304–310 (2013)
    95.55.Vj, 95.85.Ry, 98.70.Sa (all)
  7. A.D. Filonenko “Radioastronomical measurement of ultrahigh-energy cosmic particle fluxes55 741–772 (2012)
    95.55.Vj, 95.85.Bh, 96.50.S− (all)
  8. Forty years of the Institute for Nuclear Research (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 22 December 2010)54 939–974 (2011)
    01.10.Fv, 01.52.+r, 01.65.+g, 14.60.Pq, 14.60.−z, 25.30.Pt, 26.65.+t, 28.60.+s, 29.20.−c, 29.40.Ka, 32.80.Qk, 32.80.Wr, 42.55.−f, 87.56.B−, 95.55.Vj, 96.50.sb, 96.50.sh, 96.60.Vg (all)
  9. V.N. Gavrin “The Russian-American gallium experiment SAGE54 941–949 (2011)
    26.65.+t, 95.55.Vj, 96.60.Vg (all)
  10. G.V. Domogatsky “BAIKAL neutrino experiment54 949–954 (2011)
    29.40.Ka, 95.55.Vj (all)
  11. I.I. Tkachev “Telescope Array Observatory observations of the Greisen—Zatsepin—Kuzmin effect54 954–961 (2011)
    95.55.Vj, 96.50.sb, 96.50.sh (all)
  12. G.A. Gusev, B.N. Lomonosov et alIce satellites of planets of the Solar System and the on-orbit radio detection of ultrahigh-energy particles53 915–921 (2010)
    95.55.Vj, 95.85.Ry, 96.50.S− (all)
  13. A.B. Aleksandrov, A.V. Bagulya et alCharge spectrum of galactic cosmic ray nuclei as measured in meteorite olivines53 805–808 (2010)
    21.10.Ft, 26.40.+r, 95.55.Vj, 96.30.Za, 96.50.sb (all)
  14. G.T. Zatsepin, T.M. Roganova “Cosmic ray investigations52 1139–1146 (2009)
    01.30.Bb, 01.65.+g, 95.55.Vj, 96.50.S− (all)
  15. S.A. Voronov, S.V. Borisov, A.V. Karelin “Electron-proton separation in calorimetry experiments directly measuring the composition and energy spectrum of cosmic rays52 879–890 (2009)
    29.40.Vj, 95.40.+s, 95.55.Vj (all)
  16. O.G. Ryazhskaya “Neutrinos from stellar core collapses: present status of experiments49 1017–1027 (2006)
    95.55.Vj, 95.85.Ry, 97.60.−s (all)
  17. V.A. Ryabov “Ultrahigh-energy neutrinos from astrophysical sources and superheavy particle decays49 905–936 (2006)
    12.60.−i, 13.15.+g, 95.55.Vj, 95.85.Ry, 96.50.S− (all)
  18. V.L. Ginzburg “The origin of cosmic rays (Forty years later)36 (7) 587–591 (1993)
    98.70.Sa, 96.50.sb, 96.50.sd, 98.70.Dk (all)
  19. S.T. Belyaev, S.S. Gershtein et alIsai Izrailevich Gurevich (on his eightieth birthday)35 (8) 723–724 (1992)
    01.60.+q, 96.50.sb, 21.65.+f, 14.60.Lm, 13.40.Em, 28.41.Te (all)
  20. I.V. Andreev, V.L. Ginzburg et alEvgenii L’vovich Feinberg (on his eightieth birthday)35 (6) 533–534 (1992)
    01.60.+q, 23.40.−s, 29.30.Hs, 96.50.sb (all)
  21. G.V. Domogatskii, G.T. Zatsepin et alAleksandr Evgen’evich Chudakov (on his seventieth birthday)34 (7) 637–638 (1991)
    01.60.+q, 96.50.sb, 13.85.−t, 41.60.Bq (all)
  22. A.D. Erlykin, E.A. Mamidzhanyan “Autumn school ’Interactions of hadrons at super-accelerator energies’34 (4) 334–339 (1991)
    01.40.E−, 29.40.Mc, 96.50.sd, 13.60.Hb, 96.50.sb (all)
  23. B.A. Trubnikov “On the possible generation of cosmic rays in plasma pinches33 (12) 1061–1071 (1990)
    98.70.Sa, 96.50.sb, 96.50.Tf, 52.40.Kh, 94.05.Jq (all)
  24. A.D. Erlykin, E.A. Mamidzhanyan, V.A. Tsarev “Autumn school ’Interaction of hadrons at above-accelerator energies’32 380–383 (1989)
    96.50.sb, 96.50.sd, 97.60.Bw, 98.62.Ra, 01.40.E− (all)
  25. V.L. Ginzburg “Astrophysical aspects of cosmic-ray research (first 75 years and outlook for the future)31 491–510 (1988)
    96.50.sb, 98.70.Sa, 98.80.−k, 01.30.Cc (all)
  26. G.B. Khristiansen “Prospects for studying cosmic rays at ultrahigh energies (1015-1021 eV)30 1110–1112 (1987)
    96.50.sb, 98.70.Vc, 96.50.sd, 98.70.Sa (all)
  27. G.T. Zatsepin, Yu.A. Nechin, G.B. Khristiansen “Use of the magnetic induction of iron in cosmic-ray and high-energy physics30 1007–1008 (1987)
    41.20.Gz, 75.60.Ej, 96.50.sb, 96.50.sd (all)
  28. V.L. Ginzburg, M.A. Markov et alGeorgii Timofeevich Zatsepin (On his seventieth birthday)30 441–442 (1987)
    01.60.+q, 96.50.sd, 96.50.sb, 95.30.Cq, 96.60.Jw, 26.65.+t (all)
  29. A.P. Aleksandrov, V.A. Ambartsumyan et alAnatolii Alekseevich Logunov (On his sixtieth birthday)30 290–292 (1987)
    01.60.+q, 11.10.Hi, 11.10.Gh, 96.50.sb, 13.75.Cs (all)
  30. S.P. Mikheev, A.Yu. Smirnov “Neutrino oscillations in a medium with variable density29 1155–1157 (1986)
    14.60.Lm, 14.60.Pq, 96.50.Vg, 96.50.sb (all)
  31. M.B. Voloshin, M.I. Vysotskii, L.B. Okun’ “Possible electromagnetic properties of the neutrino and variations of the solar neutrino flux29 1070–1070 (1986)
    14.60.Lm, 96.50.sb, 96.50.Vg, 13.40.Em, 11.30.Ly, 97.20.−w (all)
  32. V.S. Berezinskii “High energy neutrino astrophysics28 728–730 (1985)
    96.50.sb, 97.60.Gb, 13.75.Cs, 97.60.Bw, 97.10.Cv, 97.20.Li (all)
  33. Yu.G. Abov, V.V. Vladimirskii et alAleksandr Ovseevich Vaisenberg (Obituary)28 733–734 (1985)
    01.60.+q, 96.50.sb, 13.20.Cz, 14.40.Aq, 13.35.Bv, 14.60.Ef (all)
  34. L.I. Dorman, I.Ya. Libin “Short-period variations in cosmic-ray intensity28 233–256 (1985)
    98.70.Sa, 96.50.sh, 96.50.Bh, 96.50.Ci, 96.60.Vg (all)
  35. G.A. Askar’yan “Investigation of the Earth by means of neutrinos. Neutrino geology27 896–900 (1984)
    96.50.sb, 91.60.Pn (all)
  36. A.K. Likhoded “Tenth All-Union School on Inelastic Interactions at High Energies27 647–648 (1984)
    01.40.E−, 96.50.sb, 11.30.Rd, 96.50.sd, 25.40.−h, 24.85.+p (all)
  37. G.A. Gusev, I.M. Zheleznykh “On the possibility of detection of neutrinos and muons on the basis of radio radiation of cascades in natural dielectric media (antarctic ice sheet and so forth)27 550–552 (1984)
    96.50.sd, 96.50.sb, 95.55.Vj, 14.80.Hv, 14.80.Ly (all)
  38. V.L. Ginzburg “The origin of Cosmic Rays (Present State of the Problem)18 795–796 (1975)
    01.10.Fv, 96.50.sb, 98.70.Sa, 97.60.Bw (all)
  39. G.B. Zhdanov “Errata to the article by G. B. Zhdanov, ’Search for Transuranium Elements,’ Vol. 16, No. 516 944–944 (1974)
    25.85.Ca, 21.60.Cs, 27.90.+b, 96.50.sb, 21.10.Ky, 23.60.+e (all)
  40. G.B. Zhdanov “Search for transuranium elements (methods, results, and prospects)16 642–657 (1974)
    25.85.Ca, 21.60.Cs, 27.90.+b, 96.50.sb, 21.10.Ky, 23.60.+e (all)
  41. I.L. Rozental’ “Interaction of cosmic muons of high energy11 49–65 (1968)
    96.50.sb, 95.30.Cq, 96.60.Vg, 14.40.Aq (all)
  42. E.L. Feinberg “The problem of quarks in cosmic rays10 256–261 (1967)
    96.50.sb, 14.65.−q, 11.30.Ly, 95.30.Cq (all)
  43. D.I. Blokhintsev “High-energy physics and the fundamental principles of modern theory8 612–613 (1966)
    96.50.sb, 96.50.Vg, 13.85.Dz, 13.60.Fz, 11.10.−z, 11.30.Er (all)
  44. B.M. Pontekorvo “Elementary particle physics is expensive: is it necessary?8 617–618 (1966)
    14.20.Jn, 96.50.sb, 25.30.Mr, 12.39.−x, 95.30.Cq (all)
  45. V.L. Ginzburg, S.I. Syrovatskii “Origin of cosmic rays9 223–235 (1966)
    96.50.sb, 95.30.Qd, 98.54.Gr, 97.60.Bw (all)
  46. V.L. Ginzburg, L.V. Kurnosova et alSoviet satellite and rocket investigations of the nuclear component of cosmic rays7 230–269 (1964)
    96.50.sb, 98.70.Sa, 98.70.Vc, 98.38.Am, 95.55.−n (all)
  47. S.I. Nikol’skii “Extensive air showers of cosmic radiation5 849–877 (1963)
    96.50.sd, 96.50.sb, 98.70.Vc (all)
  48. V.L. Ginzburg “Cosmic rays on Earth and in the Universe4 553–575 (1962)
    96.50.sb, 96.50.Vg, 94.20.wq, 94.30.Xy, 98.70.Sa (all)
  49. N.A. Dobrotin, N.L. Grigorov et alSERGEĬ NIKOLAEVICH VERNOV (on his fiftieth birthday)3 810–812 (1961)
    01.60.+q, 96.50.sd, 96.50.sb (all)
  50. V.L. Ginzburg, S.I. Syrovatskii “Present status of the question of the origin of cosmic rays3 504–541 (1961)
    96.50.sb, 96.50.Dj, 97.60.Bw, 96.60.Q−, 98.70.Sa (all)
  51. N.A. Dobrotin “International cosmic ray conference2 974–986 (1960)
    98.70.Sa, 96.50.sd, 96.50.sb (all)
  52. G.G. Getmantsev, V.L. Ginzburg, I.S. Shklovskii “Radio astronomical investigations with the aid of artificial satellites1 65–67 (1958)
    95.40.+s, 98.70.Vc, 96.50.sb (all)
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