PACS numbers

52.25.Xz Magnetized plasmas 94.30.C− Magnetospheric configuration and dynamics 95.30.Qd Magnetohydrodynamics and plasmas
  1. V.S. Beskin “Radio pulsars --- already fifty years!61 353–380 (2018)
    01.65.+g, 95.30.Qd, 97.60.Gb (all)
  2. D.A. Dolgolenko, Yu.A. Muromkin “On separation of mixtures of chemical elements in plasma60 994–1017 (2017)
    28.41.Kw, 52.25.Xz, 52.30.−q, 52.75.−d (all)
  3. 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)
  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. V.S. Beskin “Magnetohydrodynamic models of astrophysical jets53 1199–1233 (2010)
    95.30.Qd, 97.60.Gb, 97.60.Lf, 98.62.Nx (all)
  6. D.A. Dolgolenko, Yu.A. Muromkin “Plasma isotope separation based on ion cyclotron resonance52 345–357 (2009)
    28.60.+s, 52.20.−j, 52.25.Xz (all)
  7. 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)
  8. V.S. Beskin “Axisymmetric steady flows in astrophysics46 1209–1214 (2003)
    04.70.−s, 95.30.Qd, 97.10.Gz (all)
  9. V.S. Beskin “Axisymmetric stationary flows in compact astrophysical objects40 659–688 (1997)
    95.30.Lz, 95.30.Qd (all)
  10. V.V. Zheleznyakov “Astrophysical plasma in extreme conditions40 438–440 (1997)
    95.30.-b, 95.30.Qd
  11. 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)
  12. A.I. Morozov “Development of the principles of a quasi-steady-state plasma accelerator with an intrinsic magnetic field with a power of 109-1011 W33 (7) 576–577 (1990)
    52.59.−f, 52.65.Kj, 52.25.Xz, 52.55.Fa, 52.30.−q (all)
  13. 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)
  14. 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)
  15. 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)
  16. 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)
  17. 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)
  18. 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)
  19. 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)
  20. 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)
  21. 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)
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