PACS numbers

02.50.−r Probability theory, stochastic processes, and statistics 05.40.Fb Random walks and Levy flights 98.70.Sa Cosmic rays
  1. A.M. Bykov “Sources of high-energy cosmic radiation67 (4) (2024)
    95.30.−k, 98.70.Rz, 98.70.Sa (all)
  2. Yu.V. Bogomolov, V.V. Alekseev et alReview of unfolding methods66 628–642 (2023)
    02.50.−r, 02.60.−x, 96.50.S−, 96.50.sb (all)
  3. V.V. Uchaikin, A.D. Erlykin, R.T. Sibatov “Nonlocal (fractional-differential) model of cosmic ray transport in the interstellar medium66 221–262 (2023)
    02.50.−r, 05.40.Fb, 98.70.Sa (all)
  4. Yu.V. Stenkin “The LHAASO project: first results and prospects65 980–985 (2022)
    96.50.S−, 96.50.sd, 98.70.Sa (all)
  5. M.I. Panasyuk, L.I. Miroshnichenko “Particle acceleration in space: a universal mechanism?65 379–405 (2022)
    26.40.+r, 96.50.Vg, 98.70.Sa (all)
  6. M.I. Panasyuk “Greisen—Zatsepin—Kuzmin effect: top—down and bottom—up view61 903–911 (2018)
    98.70.Sa
  7. A.M. Bykov “Astrophysical objects with extreme energy release: observations and theory61 805–818 (2018)
    95.30.−k, 97.60.Bw, 98.70.Sa (all)
  8. S.K. Nechaev, K. Polovnikov “Rare-event statistics and modular invariance61 99–104 (2018)
    02.30.−f, 02.50.−r, 05.40.−a (all)
  9. I.V. Galaktionov “Search for antimatter and dark matter, precision studies of the cosmic rays fluxes on the international space station. AMS experiment. Results of four year exposure60 40–57 (2017)
    13.85.Tp, 14.60.−z, 29.30.−h, 75.50.Ww, 95.30.−k, 95.55.−n, 96.50.S−, 97.60.−s, 98.58.Mj, 98.70.Sa (all)
  10. A.D. Filonenko “Radio emission of extensive air showers58 633–669 (2015)
    95.55.Vj, 98.70.Sa (all)
  11. Yu.E. Kuzovlev “Why nature needs 1/f-noise58 719–729 (2015)
    05.20.Jj, 05.40.Fb (all)
  12. A. Ruzmaikin “Climate as a game of chance57 280–291 (2014)
    02.50.−r, 05.45.−a, 92.05.Df (all)
  13. V.V. Uchaikin “Fractional phenomenology of cosmic ray anomalous diffusion56 1074–1119 (2013)
    02.50.−r, 05.40.−a, 98.70.Sa (all)
  14. 120 anniversary of the birth of Academician D V Skobel’tsyn (Joint meeting of the scientific session of the Physical Sciences Division of the Russian Academy of Sciences and the Research Councils of the P N Lebedev Physical Institute of the Russian Academy of Sciences and of the D V Skobel’tsyn Institute of Nuclear Physics of M V Lomonosov Moscow State University, 28 November 2012)56 401–422 (2013)
    01.10.Fv, 01.60.+q, 01.65.+g, 25.10.+s, 41.60.Ap, 41.60.Cr, 98.70.Sa (all)
  15. G.A. Mesyats “Academician D V Skobel’tsyn and LPI56 401–404 (2013)
    01.60.+q, 01.65.+g, 98.70.Sa (all)
  16. V.A. Sadovnichy “Academician D V Skobel’tsyn and Moscow University56 404–406 (2013)
    01.60.+q, 01.65.+g, 98.70.Sa (all)
  17. I.N. Toptygin “The Petersburg period in the life and scientific work of D V Skobel’tsyn56 417–422 (2013)
    01.60.+q, 01.65.+g, 98.70.Sa (all)
  18. O.G. Ryazhskaya “On experiments in Underground Physics56 296–304 (2013)
    01.65.+g, 26.65.+t, 98.70.Sa (all)
  19. 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)
  20. Econophysics and evolutionary economics (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 2 November 2010)54 729–761 (2011)
    01.10.Fv, 02.50.−r, 05.40.−a, 05.45.Df, 89.65.Gh, 89.75.−k (all)
  21. A.Yu. Yudanov “High-growth firms in Russia: experimental data and prospects for the econophysical simulation of economic modernization54 733–737 (2011)
    02.50.−r, 89.65.Gh (all)
  22. P.V. Vidov, M.Yu. Romanovsky “Nonclassical random walks and the phenomenology of fluctuations of securities returns in the stock market54 749–753 (2011)
    02.50.−r, 89.65.Gh (all)
  23. A. Loskutov “Fascination of chaos53 1257–1280 (2010)
    02.50.−r, 05.45.−a, 47.52.+j (all)
  24. K.V. Ptitsyna, S.V. Troitsky “Physical conditions in potential accelerators of ultrahigh energy cosmic rays: updated Hillas plot and radiation-loss constraints53 691–701 (2010)
    98.54.−h, 98.62.En, 98.70.Sa (all)
  25. R.T. Sibatov, V.V. Uchaikin “Fractional differential approach to dispersive transport in semiconductors52 1019–1043 (2009)
    05.40.Fb, 72.20.−i, 73.40.−c (all)
  26. V.S. Ptuskin “On the origin of galactic cosmic rays50 534–540 (2007)
    01.10.Fv, 96.50.S−, 98.70.Sa (all)
  27. A.A. Andronov, V.L. Bratman et alJoint meeting of the Editorial Board of the Journal ’Izvestiya Vuzov. Radiofizika’ and the Scientific Council of the Institute of Applied Physics of the Russian Academy of Sciences dedicated to the ninetieth birthday of Vitalii Lazarevich Ginzburg (4 October 2006)50 301–303 (2007)
    41.20.Jb, 41.60.Cr, 42.25.Ja, 52.35.Mw, 52.59.−f, 84.40.Ik, 87.10.+e, 94.20.−y, 96.50.S−, 98.70.Sa (all)
  28. E.V. Derishev, V.V. Kocharovsky, V.V. Kocharovskii “Cosmic accelerators for ultrahigh-energy particles50 308–315 (2007)
    96.50.S−, 98.70.Sa (all)
  29. V.S. Anishchenko, T.E. Vadivasova et alStatistical properties of dynamical chaos48 151–166 (2005)
    02.50.−r, 05.45.−a, 47.52.+j (all)
  30. V.V. Uchaikin “Self-similar anomalous diffusion and Levy-stable laws46 821–849 (2003)
    02.50.−r, 05.40.Fb, 05.40.Jc (all)
  31. V.I. Klyatskin “Clustering and diffusion of particles and passive tracer density in random hydrodynamic flows46 667–688 (2003)
    02.50.−r, 05.40.−a, 05.45.−a (all)
  32. V.I. Klyatskin, K.V. Koshel’ “Simple example of the development of cluster structure of a passive tracer field in random flows43 717–723 (2000)
    02.50.−r, 05.40.-j, 05.45.+b
  33. V.V. Lobzin, V.R. Chechetkin “Order and correlations in genomic DNA sequences. The spectral approach43 55–78 (2000)
    02.50.−r, 05.10.−a, 87.10.+e, 87.14.Gg (all)
  34. V.I. Klyatskin, D. Gurarie “Coherent phenomena in stochastic dynamical systems42 165 (1999)
    02.50.−r, 05.40.-j, 05.45.+b, 42.50.−p (all)
  35. V.L. Ginzburg “Cosmic ray astrophysics (history and general review)39 155–168 (1996)
    98.70.Sa
  36. V.V. Mityugov “The tree of paradox36 (8) 744–753 (1993)
    03.65.Ud, 03.65.Ta, 05.40.Fb (all)
  37. 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)
  38. V.N. Tutubalin “Probability, computers, and the processing of experimental data36 (7) 628–641 (1993)
    01.40.gb, 01.50.ht, 02.50.−r, 06.20.Dk (all)
  39. A.V. Andreev “Probability, statistical optics, and data testing35 (1) 53–53 (1992)
    01.30.Vv, 02.50.−r, 05.40.−a (all)
  40. V.I. Alkhimov “The self-avoiding walk problem34 (9) 804–816 (1991)
    05.40.Fb, 64.60.Ak, 64.60.Fr (all)
  41. 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)
  42. 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)
  43. 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)
  44. 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)
  45. 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)
  46. 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)
  47. 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)
  48. G.B. Khristiansen “Apparatus for studying extremely high energy cosmic rays30 539–541 (1987)
    98.70.Sa, 95.85.Ry (all)
  49. E.A. Mamidzhanyan, S.I. Nikol’skii “Possibility of experimental ultrahigh-energy gamma-ray astronomy30 542–543 (1987)
    98.70.Rz, 98.70.Sa, 97.60.Gb, 98.54.Aj, 98.58.Mj, 96.50.sd (all)
  50. 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)
  51. V.L. Ginzburg “The origin of Cosmic Rays (Present State of the Problem)17 795–796 (1975)
    01.10.Fv, 96.50.sb, 98.70.Sa, 97.60.Bw (all)
  52. I.A. Aslanov, V.L. Khokhlova, W. Schoneich “Properties of Magnetic Stars from Spectral and Photometric Investigations17 803–804 (1975)
    98.70.Rz, 98.70.Sa, 98.38.Mz (all)
  53. A.M. Gal’per, V.G. Kirillov-Ugryumov, B.I. Luchkov “Observational gamma astronomy17 186–198 (1974)
    98.70.Rz, 98.70.Sa, 98.80.Es, 97.60.Gb (all)
  54. V.N. Sazonov “Circular polarization of radiation from cosmic objects15 822–830 (1973)
    98.54.Aj, 96.30.Kf, 97.20.Rp, 98.70.Dk, 98.70.Sa (all)
  55. V.F. Turchin, V.P. Kozlov, M.S. Malkevich “The use of mathematical-statistics methods in the solution of incorrectly posed problems13 681–703 (1971)
    02.30.Zz, 02.50.−r (all)
  56. I.S. Shklovskii “Discovery of pulsed sources of cosmic radio emission with strictly periodic variation of the flux11 435–436 (1968)
    98.70.Dk, 98.70.Sa, 98.70.Vc, 97.60.Gb (all)
  57. V.L. Ginzburg “Powerful X-ray emission of radio galaxies9 543–550 (1967)
    98.54.Gr, 98.70.Qy, 98.70.Sa (all)
  58. V.L. Ginzburg, S.I. Syrovatskii “Some problems of gamma and X-ray astronomy7 696–720 (1965)
    98.70.Qy, 98.70.Rz, 98.70.Sa (all)
  59. 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)
  60. 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)
  61. 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)
  62. F.G. Bass, S.Ya. Braude et alFluctuations of electromagnetic waves in the troposphere in the presence of separation boundaries4 51–69 (1961)
    92.60.Ta, 41.20.Jb, 92.60.hk, 02.50.−r (all)
  63. N.A. Dobrotin “International cosmic ray conference2 974–986 (1960)
    98.70.Sa, 96.50.sd, 96.50.sb (all)
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