PACS numbers

52.70.Kz Optical (ultraviolet, visible, infrared) measurements
  1. L.M. Biberman, B.A. Veklenko et alValentin Aleksandrovich Fabrikant (Obituary)34 (6) 549–550 (1991)
    01.60.+q, 52.25.Os, 52.70.Kz, 52.80.−s, 52.20.−j, 52.38.Bv (all)
  2. A.P. Aleksandrov, S.T. Belyaev et alYurii Efremovich Nesterikhin (on his sixtieth birthday)33 (10) 870–871 (1990)
    01.60.+q, 52.35.Tc, 52.50.Lp, 52.70.Kz, 89.20.Bb (all)
  3. Yu.S. Protasov “First All-Union Symposium on Radiation Plasmodynamics33 (7) 583–584 (1990)
    52.35.Tc, 52.25.Kn, 52.70.Kz, 52.50.Dg, 52.30.−q, 01.30.Cc (all)
  4. A.N. Zaidel’ “Application of holographic interferometry for plasma diagnostics29 447–466 (1986)
    42.40.Kw, 42.70.−a, 52.70.Kz (all)
  5. V.N. Ochkin, N.G. Preobrazhenskii et alOptogalvanic effect in plasmas and gases29 260–280 (1986)
    52.70.Kz, 52.80.Hc, 33.20.Vq, 52.80.Pi, 32.80.Rm (all)
  6. V.V. Pikalov, N.G. Preobrazhenskii “Computer-aided tomography and physical experiment26 974–990 (1983)
    42.30.Va, 06.70.Hs, 93.85.+q, 52.70.Kz (all)
  7. N.B. Delone “Elementary nonlinear optical phenomena16 749–752 (1974)
    42.65.−k, 32.80.Rm, 52.70.Kz, 32.80.Cy, 33.80.Rv (all)
  8. Ya.S. Bobovich “Laser spectroscopy utilizing spontaneous raman scattering of weakly interacting molecules and its applications15 671–687 (1973)
    33.20.Fb, 33.20.Sn, 33.20.Vq, 52.70.Kz, 92.60.H− (all)
  9. M.P. Vanyukov, A.A. Mak “High-intensity pulsed light sources1 137–155 (1958)
    52.70.Kz, 42.72.−g, 52.80.Mg, 52.80.Qj, 52.35.Tc (all)
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