Methods of Studying the Spectral Composition of Scattered Light

  • Academician D. V. Skobel’tsyn
Part of the The Lebedev Physics Institute Series book series (LPIS, volume 39)


In studying the spectral intensity distribution in the wing of the Rayleigh line, we used a photoelectric method of recording the spectra. As spectral apparatus we used a DFS-12 diffraction spectrograph with two 600 lines/mm replica gratings working in the second order. The apparatus had a dispersion of 4.6 Å/mm. For slits of ~ 2–4 μ the half-width of the apparatus function, together with the intrinsic worth of the Hg 4358 A line, was ~0.6 cm-1. The main arrangement of the apparatus is shown in Fig. 1.


Exciting Light Aperture Angle Rayleigh Line Apparatus Function Exciting Line 
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Copyright information

© Consultants Bureau 1969

Authors and Affiliations

  • Academician D. V. Skobel’tsyn
    • 1
  1. 1.P. N. Lebedev Physics InstituteAcademy of Sciences of the USSRMoscowRussia

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