PACS numbers

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. 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. 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)
  4. V.S. Beskin “Magnetohydrodynamic models of astrophysical jets53 1199–1233 (2010)
    95.30.Qd, 97.60.Gb, 97.60.Lf, 98.62.Nx (all)
  5. 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)
  6. V.S. Beskin “Axisymmetric steady flows in astrophysics46 1209–1214 (2003)
    04.70.−s, 95.30.Qd, 97.10.Gz (all)
  7. V.S. Beskin “Axisymmetric stationary flows in compact astrophysical objects40 659–688 (1997)
    95.30.Lz, 95.30.Qd (all)
  8. V.V. Zheleznyakov “Astrophysical plasma in extreme conditions40 438–440 (1997)
    95.30.-b, 95.30.Qd
  9. 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)
  10. 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)
  11. 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)
  12. 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)
  13. 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)
  14. 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)
  15. 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)
  16. 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)
  17. 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)
  18. 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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