PACS numbers

02.50.−r Probability theory, stochastic processes, and statistics 02.60.−x Numerical approximation and analysis 96.50.sb Composition, energy spectra and interactions
  1. 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)
  2. 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)
  3. S.K. Nechaev, K. Polovnikov “Rare-event statistics and modular invariance61 99–104 (2018)
    02.30.−f, 02.50.−r, 05.40.−a (all)
  4. A. Ruzmaikin “Climate as a game of chance57 280–291 (2014)
    02.50.−r, 05.45.−a, 92.05.Df (all)
  5. V.V. Uchaikin “Fractional phenomenology of cosmic ray anomalous diffusion56 1074–1119 (2013)
    02.50.−r, 05.40.−a, 98.70.Sa (all)
  6. 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)
  7. 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)
  8. 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)
  9. 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)
  10. 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)
  11. A. Loskutov “Fascination of chaos53 1257–1280 (2010)
    02.50.−r, 05.45.−a, 47.52.+j (all)
  12. 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)
  13. 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)
  14. V.V. Uchaikin “Self-similar anomalous diffusion and Levy-stable laws46 821–849 (2003)
    02.50.−r, 05.40.Fb, 05.40.Jc (all)
  15. 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)
  16. I.M. Dremin, O.V. Ivanov, V.A. Nechitailo “Wavelets and their uses44 447–478 (2001)
    02.60.−x, 02.70.−c, 05.40.−a, 87.57.−s (all)
  17. 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
  18. 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)
  19. 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)
  20. 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)
  21. 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)
  22. 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)
  23. 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)
  24. A.V. Andreev “Probability, statistical optics, and data testing35 (1) 53–53 (1992)
    01.30.Vv, 02.50.−r, 05.40.−a (all)
  25. 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)
  26. 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)
  27. 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)
  28. 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)
  29. 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)
  30. 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)
  31. 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)
  32. 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)
  33. 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)
  34. 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)
  35. 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)
  36. 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)
  37. 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)
  38. G.A. Askar’yan “Investigation of the Earth by means of neutrinos. Neutrino geology27 896–900 (1984)
    96.50.sb, 91.60.Pn (all)
  39. 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)
  40. 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)
  41. 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)
  42. 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)
  43. 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)
  44. G.M. Zaslavskii, B.V. Chirikov “Stochastic instability of non-linear oscillations14 549–568 (1972)
    02.50.Ey, 05.45.Xt, 02.50.Cw, 02.60.−x (all)
  45. 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)
  46. 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)
  47. 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)
  48. 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)
  49. 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)
  50. 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)
  51. 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)
  52. S.I. Nikol’skii “Extensive air showers of cosmic radiation5 849–877 (1963)
    96.50.sd, 96.50.sb, 98.70.Vc (all)
  53. 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)
  54. 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)
  55. 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)
  56. 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)
  57. N.A. Dobrotin “International cosmic ray conference2 974–986 (1960)
    98.70.Sa, 96.50.sd, 96.50.sb (all)
  58. 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)
© 1918–2024 Uspekhi Fizicheskikh Nauk
Email: ufn@ufn.ru Editorial office contacts About the journal Terms and conditions