PACS numbers

95.30.Gv Radiation mechanisms; polarization
  1. V.S. Beskin, Ya.N. Istomin, A.A. Philippov “Radio pulsars: the search for truth56 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 type46 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 inhomogeneities45 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 astrophysics32 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 Mars9 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)8 674–701 (1966)
    98.70.Vc, 96.60.Tf, 95.30.Gv, 41.60.Ap, 95.30.Qd (all)
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