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Issue 11, 2024
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PACS numbers

52.65.Kj Magnetohydrodynamic and fluid equation
  1. V.D. Kuznetsov, A.I. Osin “Heliophysics: from observations to models and applications” Phys. Usp. 63 812–817 (2020)
    52.35.Bj, 52.35.Tc, 52.65.Kj (all)
  2. E.P. Kurbatov, A.G. Zhilkin, D.V. Bisikalo “Modified magnetohydrodynamics model including wave turbulence: astrophysical applications” Phys. Usp. 60 798–817 (2017)
    52.30.Cv, 52.35.Bj, 52.35.Ra, 52.65.Kj, 95.30.Qd, 94.05.Lk, 97.80.Gm (all)
  3. A.A. Chernyshov, K.V. Karelsky, A.S. Petrosyan “Subgrid-scale modeling for the study of compressible magnetohydrodynamic turbulence in space plasmas” Phys. Usp. 57 421–452 (2014)
    47.27.E−, 47.27.ep, 47.27.Gs, 52.35.Ra, 52.65.Kj (all)
  4. B.A. Trubnikov “Constrictions in a relativistic pinch with a longitudinal magnetic field” Sov. Phys. Usp. 34 (11) 1018–1020 (1991)
    52.27.Ny, 52.58.Lq, 52.65.Kj, 52.80.−s (all)
  5. 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 W” Sov. Phys. Usp. 33 (7) 576–577 (1990)
    52.59.−f, 52.65.Kj, 52.25.Xz, 52.55.Fa, 52.30.−q (all)
  6. E.G. Berezhko, G.F. Krymskii “Acceleration of cosmic rays by shock waves” Sov. Phys. Usp. 31 27–51 (1988)
    52.65.Kj, 95.30.Qd, 96.50.Fm, 97.60.Bw, 98.70.Sa (all)
  7. E.G. Berezhko, G.F. Krymskii “Acceleration of cosmic rays by shock waves” Sov. Phys. Usp. 31 27–51 (1988)
    96.50.Fm, 98.70.Sa, 97.60.Bw, 52.65.Kj, 95.30.Qd (all)
  8. S.M. Osovets “Dynamic methods of confinement and stabilization of hot plasma” Sov. Phys. Usp. 17 239–262 (1974)
    52.58.Lq, 52.25.−b, 52.35.Py, 52.30.−q, 52.65.Kj (all)
  9. M.A. Gintsburg “Nonlinear Waves in Cosmic Plasma” Sov. Phys. Usp. 12 692–692 (1970)
    96.50.Tf, 52.30.Cv, 52.65.Kj, 52.35.Mw (all)
  10. L.A. Artsimovich “Present state of research in controlled thermonuclear reactions” Sov. Phys. Usp. 5 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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