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Diffuse Reflection and Transmission by Non-Coherently Scattering Media

Published online by Cambridge University Press:  25 April 2016

R. B. T. Black
R. B. T. Black*
Affiliation:
Department of Applied Mathematics, University of Sydney
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Extract

It has become recognized that the dominant mechanism in the formation of the cores of resonance lines in the solar spectrum is non-coherent scattering, e.g., Thomas (1957). A study, preliminary to the theoretical investigation of the spectra of chromospheric structures, is the evaluation of the effect of diffuse reflection and transmission by non-coherently scattering media.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 1 , January 1967 , pp. 11
Copyright
Copyright © Astronomical Society of Australia 1967

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References

Giovanelli, R. G., 1966.—Aust. J. Thys. (to be published).Google Scholar
Thomas, R. N., 1957.—Ap. J., 125, 260.CrossRefGoogle Scholar