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  • Access by Xinjiang University

On the Diffusion of Imprisoned Resonance Radiation

Frank N. Edmonds, Jr.

  • Yerkes Observatory, University of Chicago, Williams Bay, Wisconsin

Phys. Rev. 78, 424 – Published 15 May, 1950

DOI: https://doi.org/10.1103/PhysRev.78.424

Abstract

The solution of the problem of diffusion of imprisoned resonance radiation obtained by Chandrasekhar is worked out in detail in the second approximation. Decay constants, characteristic roots and eigenfunction coefficients necessary for an explicit solution are tabulated for both large and small optical thicknesses. A comparison is made between computed and measured decay constants for the Hg 2537A resonance line.

References (8)

  1. E. A. Milne, J. Math. Soc. London 1, 40 (1926)
  2. S. Chandrasekhar, Radiative Transfer (Clarendon Press, Oxford, 1950), p. 354
  3. M. W. Zemansky, Phys. Rev. 29, 513 (1927)
  4. Alpert, McCoubray, and Holstein, Phys. Rev. 76, 1257 (1949)
  5. H. Zanstra, Bull. Astronom. Insts. Netherlands X1, No. 401 (1949)
  6. M. W. Zemansky, Phys. Rev. 42, 843 (1932)
  7. C. Kenty, Phys. Rev. 42, 823 (1932)
  8. T. Holstein, Phys. Rev. 72, 1212 (1947)

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