PACS numbers

95.30.Qd Magnetohydrodynamics and plasmas 96.50.sb Composition, energy spectra and interactions 97.60.Bw Supernovae 98.54.Gr Radio galaxies
  1. V.S. Beskin “Radio pulsars --- already fifty years!61 353–380 (2018)
    01.65.+g, 95.30.Qd, 97.60.Gb (all)
  2. E.P. Kurbatov, A.G. Zhilkin, D.V. Bisikalo “Modified magnetohydrodynamics model including wave turbulence: astrophysical applications60 798–817 (2017)
    52.30.Cv, 52.35.Bj, 52.35.Ra, 52.65.Kj, 95.30.Qd, 94.05.Lk, 97.80.Gm (all)
  3. G.S. Bisnovatyi-Kogan, S.G. Moiseenko “Gravitational waves and core-collapse supernovae60 843–850 (2017)
    04.80.Nn, 95.85.Sz, 97.60.Bw, 97.60.Lf (all)
  4. L.M. Zelenyi, H.V. Malova et alThin current sheets: from the work of Ginzburg and Syrovatskii to the present day59 1057–1090 (2016)
    52.25.Xz, 94.30.C−, 95.30.Qd (all)
  5. P.V. Baklanov, S.I. Blinnikov et alITEP's achievements in astrophysics59 796–806 (2016)
    01.65.+g, 97.60.Bw, 97.80.−d (all)
  6. B.P. Schmidt “The path to measuring an accelerating Universe56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw, 98.80.Es (all)
  7. A.G. Riess “My path to the accelerating Universe56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw (all)
  8. S. Perlmutter “Measuring the acceleration of the cosmic expansion using supernovae56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw, 98.80.Es (all)
  9. 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)
  10. 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)
  11. V.S. Beskin “Magnetohydrodynamic models of astrophysical jets53 1199–1233 (2010)
    95.30.Qd, 97.60.Gb, 97.60.Lf, 98.62.Nx (all)
  12. V.S. Imshennik “Rotational explosion mechanism for collapsing supernovae and the two-stage neutrino signal from supernova 1987A in the Large Magellanic Cloud53 1081–1092 (2010)
    95.85.Sz, 97.60.Bw, 97.80.−d (all)
  13. V.S. Ptuskin “The origin of cosmic rays53 958–961 (2010)
    96.50.S−, 97.60.Bw, 98.62.Nx (all)
  14. 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)
  15. A.M. Bykov, I.N. Toptygin “Instabilities of a multicomponent plasma with accelerated particles and magnetic field generation in astrophysical objects50 141–174 (2007)
    52.35.−g, 52.59.−f, 95.30.Qd (all)
  16. V.S. Beskin “Axisymmetric steady flows in astrophysics46 1209–1214 (2003)
    04.70.−s, 95.30.Qd, 97.10.Gz (all)
  17. D.Yu. Tsvetkov “Type Ib/c supernovae: new observational data45 900–902 (2002)
    97.60.Bw
  18. V.S. Imshennik “Supernova explosions and historical chronology43 509–513 (2000)
    01.75.+m, 01.90.+g, 97.60.Bw, 98.58.Mj (all)
  19. N.V. Ardelyan, G.S. Bisnovatyi-Kogan, S.G. Moiseenko “Explosion mechanisms of supernovae: the magnetorotational model40 1076–1079 (1997)
    04.40.Dg, 95.30.−k, 97.60.Bw (all)
  20. V.S. Beskin “Axisymmetric stationary flows in compact astrophysical objects40 659–688 (1997)
    95.30.Lz, 95.30.Qd (all)
  21. V.V. Zheleznyakov “Astrophysical plasma in extreme conditions40 438–440 (1997)
    95.30.-b, 95.30.Qd
  22. 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)
  23. V.S. Beskin, V.I. Par’ev “Axially symmetric steady-state flows in the vicinity of a Kerr black hole and the nature of the activity of galactic nuclei36 (6) 529–539 (1993)
    98.62.Js, 95.30.Qd, 96.60.Vg, 98.54.Cm, 98.54.Aj (all)
  24. 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)
  25. 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)
  26. 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)
  27. 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)
  28. 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)
  29. V.G. Ryasnyĭ “Supernova shells33 (5) 393–395 (1990)
    97.60.Bw, 96.10.+i, 97.60.Gb, 97.60.Jd, 96.60.qe (all)
  30. V.L. Ginzburg, V.A. Dogel’ “Erratum: Some aspects of gamma-ray astronomy [Sov. Phys. Uspekhi 32, 358 (May 1989)]32 1117–1117 (1989)
    98.70.Rz, 98.70.Sa, 98.58.Db, 97.60.Bw, 98.62.Gq (all)
  31. V.L. Ginzburg, V.A. Dogel’ “Some aspects of gamma-ray astronomy32 385–415 (1989)
    98.70.Rz, 98.70.Sa, 98.58.Db, 97.60.Bw, 98.62.Gq (all)
  32. V.L. Dadykin, G.T. Zatsepin, O.G. Ryazhskaya “Events detected by underground detectors on February 23, 198732 459–468 (1989)
    97.10.Bt, 95.30.Sf, 97.60.Bw, 14.60.Lm, 29.40.Mc (all)
  33. 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)
  34. V.V. Burdyuzha “Megamasers31 763–771 (1988)
    98.38.Er, 98.54.Gr (all)
  35. N.N. Chugai “Supernova in the Large Magellanic Cloud: first year of observations31 775–776 (1988)
    97.60.Bw, 98.56.Si, 97.60.Jd, 97.10.Fy, 97.10.Ri (all)
  36. G.S. Bisnovatyi-Kogan “Gravitational collapse, neutrino radiation, and supernova light curves31 776–777 (1988)
    97.60.Bw, 95.30.Sf, 95.55.Qf, 95.75.De, 97.20.Rp, 97.10.Gz (all)
  37. 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)
  38. E.G. Berezhko, G.F. Krymskii “Acceleration of cosmic rays by shock waves31 27–51 (1988)
    52.65.Kj, 95.30.Qd, 96.50.Fm, 97.60.Bw, 98.70.Sa (all)
  39. E.G. Berezhko, G.F. Krymskii “Acceleration of cosmic rays by shock waves31 27–51 (1988)
    96.50.Fm, 98.70.Sa, 97.60.Bw, 52.65.Kj, 95.30.Qd (all)
  40. 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)
  41. 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)
  42. 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)
  43. 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)
  44. V.B. Braginskii, L.P. Grishchuk “Gravitational wave astronomy30 81–82 (1987)
    04.30.−w, 97.60.Bw, 98.80.Bp, 98.80.Cq (all)
  45. 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)
  46. 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)
  47. V.S. Beskin, A.V. Gurevich, Ya.N. Istomin “Physics of pulsar magnetospheres29 946–970 (1986)
    97.60.Gb, 97.10.Ex, 97.10.Ld, 95.30.Qd, 98.70.Dk (all)
  48. 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)
  49. 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)
  50. G.A. Askar’yan “Investigation of the Earth by means of neutrinos. Neutrino geology27 896–900 (1984)
    96.50.sb, 91.60.Pn (all)
  51. 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)
  52. 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)
  53. 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)
  54. 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)
  55. 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)
  56. P.V. Shcheglov “Astroclimatic Conditions in Central Asia and Kazakhstan14 792–794 (1972)
    97.30.Qt, 97.60.Bw, 95.75.De, 97.10.Ri, 98.80.Es, 97.10.Cv (all)
  57. A.M. Gal’per, V.G. Kirillov-Ugryumov et alThe study of cosmic γ rays14 630–654 (1972)
    98.70.Rz, 96.50.Xy, 96.60.Ub, 98.54.Gr, 98.70.Dk, 98.38.Mz (all)
  58. S.I. Vainshtein, Ya.B. Zel’dovich “Origin of Magnetic Fields in Astrophysics (Turbulent ’Dynamo’ Mechanisms)15 159–172 (1972)
    95.85.Sz, 95.30.Qd, 96.60.Hv, 97.10.Ld (all)
  59. V.L. Ginzburg “Pulsars (General Review)12 800–804 (1970)
    97.60.Gb, 97.60.Bw (all)
  60. N.S. Kardashev “Possibility of Observing Extragalactic Pulsars12 808–808 (1970)
    97.60.Gb, 97.60.Bw, 98.70.Dk, 98.54.Gr, 98.54.Aj (all)
  61. N.A. Lotova “Radioastronomical investigations of the inhomogeneous structure of the near-solar plasma11 424–434 (1968)
    96.60.P−, 96.60.Vg, 95.30.Qd, 96.50.Ci, 98.70.Dk (all)
  62. 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)
  63. V.L. Ginzburg “Powerful X-ray emission of radio galaxies9 543–550 (1967)
    98.54.Gr, 98.70.Qy, 98.70.Sa (all)
  64. Ya.B. Zel’dovich “The "hot" model of the Universe9 602–617 (1967)
    98.80.Cq, 95.30.Qd, 98.80.Es, 98.62.Ra (all)
  65. 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)
  66. V.L. Ginzburg, S.I. Syrovatskii “Cosmic magnetic bremsstrahlung (synchrotron radiation)8 674–701 (1966)
    98.70.Vc, 96.60.Tf, 95.30.Gv, 41.60.Ap, 95.30.Qd (all)
  67. Ya.B. Zel’dovich, I.D. Novikov “Relativistic astrophysics. II8 522–577 (1966)
    97.10.Kc, 97.10.Cv, 97.10.Gz, 97.60.Jd, 95.30.Qd, 98.54.Aj (all)
  68. 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)
  69. 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)
  70. 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)
  71. 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)
  72. S.I. Nikol’skii “Extensive air showers of cosmic radiation5 849–877 (1963)
    96.50.sd, 96.50.sb, 98.70.Vc (all)
  73. 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)
  74. I.S. Shklovskii “RADIO GALAXIES5 365–400 (1962)
    98.70.Dk, 95.55.Br, 98.54.Gr, 97.60.Bw (all)
  75. 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)
  76. 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)
  77. N.A. Dobrotin “International cosmic ray conference2 974–986 (1960)
    98.70.Sa, 96.50.sd, 96.50.sb (all)
  78. 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)
  79. A.M. Bykov “Astrophysical objects with extreme energy release: observations and theory”, accepted
    95.30.−k, 97.60.Bw, 98.70.Sa (all)
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