Astrophysics and Space Science

, Volume 111, Issue 1, pp 189–195 | Cite as

The ChandrasekharH-function for exponentially varying atmosphere

  • M. H. Haggag
  • H. M. Machali


The ChandrasekharH-function for exponentially-varying atmosphere is calculated. The calculations have been carried out on the assumption that the scattering function behaves also exponentially. Numerical results are given forH and for the emergent flux at the surface.


Atmosphere Emergent Flux 
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  1. Busbridge, I. W.: 1961,Astrophys. J. 133, 198.Google Scholar
  2. Garcia, R. D. M., and Siewert, C. E.: 1981,J. Quant. Spectr. Rad. Transfer 25, 277.Google Scholar
  3. Sobolev, V. V.: 1956,Soviet Phys. Dokl. 1, 747.Google Scholar
  4. Sobolev, V. V. and Loskutov, V. M.: 1976,Soviet Phys. Dokl. 20, 647.Google Scholar
  5. Ueno, S.: 1960,Astrophys. J. 132, 729.Google Scholar

Copyright information

© D. Reidel Publishing Company 1985

Authors and Affiliations

  • M. H. Haggag
    • 1
  • H. M. Machali
    • 1
  1. 1.Physics Department, Faculty of ScienceMansoura UniversityEgypt

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