PACS numbers

52.65.Kj Magnetohydrodynamic and fluid equation
  1. 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)
  2. A.A. Chernyshov, K.V. Karelsky, A.S. Petrosyan “Subgrid-scale modeling for the study of compressible magnetohydrodynamic turbulence in space plasmas57 421–452 (2014)
    47.27.E−, 47.27.ep, 47.27.Gs, 52.35.Ra, 52.65.Kj (all)
  3. B.A. Trubnikov “Constrictions in a relativistic pinch with a longitudinal magnetic field34 (11) 1018–1020 (1991)
    52.27.Ny, 52.58.Lq, 52.65.Kj, 52.80.−s (all)
  4. 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)
  5. 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)
  6. 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)
  7. S.M. Osovets “Dynamic methods of confinement and stabilization of hot plasma17 239–262 (1974)
    52.58.Lq, 52.25.−b, 52.35.Py, 52.30.−q, 52.65.Kj (all)
  8. M.A. Gintsburg “Nonlinear Waves in Cosmic Plasma12 692–692 (1970)
    96.50.Tf, 52.30.Cv, 52.65.Kj, 52.35.Mw (all)
  9. L.A. Artsimovich “Present state of research in controlled thermonuclear reactions5 1–6 (1962)
    52.35.Py, 52.75.−d, 52.55.Ez, 52.55.Hc, 25.60.Pj, 52.65.Kj (all)
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