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Raman scattering of photons in the solar interior

Published online by Cambridge University Press:  13 March 2009

V. N. Tsytovich ,
R. Bingham  and
U. de Angelis
V. N. Tsytovich
Affiliation:
Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX, U.K.
R. Bingham
Affiliation:
Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX, U.K.
U. de Angelis
Affiliation:
Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX, U.K.
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Abstract

We reconsider the transport equation in the solar interior and calculate the effects on the opacity of photon scattering near the Raman resonance. Both spontaneous and stimulated scattering on thermal photons and thermal plasmons are taken into account, and changes in opacity (with respect to previous calculations) are calculated numerically and found to be negligible with respect to relativistic corrections to photon scattering.

Type
Research Article
Information
Journal of Plasma Physics , Volume 53 , Issue 3 , June 1995 , pp. 335 - 344
Copyright
Copyright © Cambridge University Press 1995

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References

REFERENCES

Evans, D. E. & Katzenstein, J., 1969 Laser light scattering in laboratory plasmas. Rep. Prog. Phys. 32, 207.CrossRefGoogle Scholar
Tsytovich, V. N. 1970 Nonlinear Effects in Plasma. Plenum.CrossRefGoogle Scholar
Tsytovich, V. N., Bingham, R., De Angelis, U. & Forlani, A. 1995 a Collective scattering and bremsstrahlung in the solar interior. Phys. Rev. Lett. (submitted).Google Scholar
Tsytovich, V. N., Bingham, R., De Angelis, U. & Forlani, A. 1995 b Broadening of the Raman resonance in photon scattering in the solar interior. Phys. Plasmas (submitted).CrossRefGoogle Scholar