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Issue 11, 2024
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PACS numbers

82.50.Hp Processes caused by visible and UV light
  1. M.S. Murga “Evolution of carbon particles from the stage of asymptotic giant branch stars to planetary nebulae: observations, experiments, and theory” Phys. Usp. 67 961–987 (2024)
    82.33.Vx, 82.50.Hp, 95.30.Wi, 97.10.Fy, 98.38.Jw (all)
  2. G.N. Makarov “Control of the parameters and composition of molecular and cluster beams by means of IR lasers” Phys. Usp. 61 617–644 (2018)
    06.30.−k, 07.77.Gx, 33.80.−b, 36.40.−c, 41.75.Jv, 42.62.Fi, 82.50.Hp (all)
  3. G.N. Makarov “Kinetic methods for measuring the temperature of clusters and nanoparticles in molecular beams” Phys. Usp. 54 351–370 (2011)
    07.77.Gx, 36.40.−c, 36.40.Ei, 42.62.Fi, 81.07.Nb, 82.50.Hp (all)
  4. G.N. Makarov “The spectroscopy of clusters by intense pulses of VUV radiation from free electron lasers” Phys. Usp. 52 461–486 (2009)
    32.80.−t, 36.40.−c, 41.60.Cr, 42.55.Vc, 42.62.Fi, 52.50.−b, 82.50.Hp (all)
  5. G.V. Rozenberg “ÉDUARD VLADIMIROVICH SHPOL’SKIĬ (On the occasion of his seventieth birthday)” Sov. Phys. Usp. 6 157–160 (1963)
    01.60.+q, 78.55.−m, 82.50.Hp, 82.80.−d (all)
© 1918–2024 Uspekhi Fizicheskikh Nauk
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