PACS numbers

95.30.Gv Radiation mechanisms; polarization
  1. V.S. Beskin, Ya.N. Istomin, A.A. Philippov “Radio pulsars: the search for truthPhys. Usp. 56 164–179 (2013)
    52.35.−g, 95.30.Gv, 97.60.Gb (all)
  2. A.V. Stepanov “On the nature of radio emission from stars of late spectral typePhys. Usp. 46 97–102 (2003)
    95.30.Gv, 97.10.Ri, 97.80.Fk (all)
  3. K.Yu. Platonov, G.D. Fleishman “Transition radiation in media with random inhomogeneitiesPhys. Usp. 45 235–291 (2002)
    41.60.−m, 52.35.Hr, 95.30.Gv (all)
  4. A.M. Shalagin “Light-induced drift and its manifestations, particularly in astrophysicsSov. Phys. Usp. 32 281–282 (1989)
    32.80.Pj, 32.70.Jz, 95.30.Gv, 32.80.Bx, 97.30.Fi (all)
  5. A.D. Kuz’min “Results of radio observations of Mercury, Venus, and MarsSov. Phys. Usp. 9 759–766 (1967)
    96.30.Ea, 96.30.Gc, 96.30.Dz, 95.55.Jz, 95.30.Gv (all)
  6. V.L. Ginzburg, S.I. Syrovatskii “Cosmic magnetic bremsstrahlung (synchrotron radiation)Sov. Phys. Usp. 8 674–701 (1966)
    98.70.Vc, 96.60.Tf, 95.30.Gv, 41.60.Ap, 95.30.Qd (all)
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