Abstract
By performing the one-sided Laplace transform on the matrix integro-differential equation for a semi-infinite plane parallel imperfect Rayleigh scattering atmosphere we derive an integral equation for the emergent intensity matrix. Application of the Wiener-Hopf technique to this integral equation will give the emergent intensity matrix in terms of singularH-matrix and an unknown matrix. The unknown matrix has been determined considering the boundary condition at infinity to be identical with the asymptotic solution for the intensity matrix.
Similar content being viewed by others
References
Abhyankar, K. D. and Fymat, A. L.: 1970,Astron. Astrophys. 4, 101.
Case, K. M.: 1960,Ann. Phys. 9, 1.
Chandrasekhar, S.: 1950,Radiative Transfer, Oxford University Press.
Das, R. N.: 1978,Astrophys. Space Sci. 57, 429.
Domke, H.: 1971,Soviet Astron. Astrophys. J. 15, 600.
Pahor, S.: 1968,Nucl. Sci. Eng. 31, 1.
Siewert, C. E. and Frayley, K.: 1967,Ann. Phys. 43, 338.
Schnatz, T. W. and Siewert, C. E.: 1970,J. Math. Phys. 11, 2733.
Sekera, Z.: 1963, Rand Memorandum, R-413-PR (Santa Monica, Rand Corporation).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Das, R.N. Exact solution of the transport equation for imperfect rayleigh scattering in a semi-infinite atmosphere. Astrophys Space Sci 62, 143–147 (1979). https://doi.org/10.1007/BF00643908
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00643908