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2 - Classical Light Scattering Theory

Published online by Cambridge University Press:  24 February 2022

Chiao-Yao She
Affiliation:
Colorado State University
Jonathan S. Friedman
Affiliation:
Universidad Ana G. Mendez
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Summary

In Chapter 2, we present classical light scattering theory. We show the classical electric dipole and how it leads to a model of atomic polarizability and differential scattering cross section. This leads us to the two principal divisions of atomic and molecular scattering, resonant and nonresonant. From here, we close with the causes of broadening of the scattering spectrum, as compared to the laser excitation.

Type
Chapter
Information
Atmospheric Lidar Fundamentals
Laser Light Scattering from Atoms and Linear Molecules
, pp. 7 - 16
Publisher: Cambridge University Press
Print publication year: 2022

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References

Griffith, D. J. (1998). Introduction to Electrodynamics. 2nd ed. Prentice Hall.Google Scholar
Corney, A. (1977). Atomic and Laser Spectroscopy. Oxford Press.Google Scholar
She, C.-Y., Chen, H., and Krueger, D. A.. (2015). Optical processes for middle atmospheric Doppler lidars: Cabannes scattering and laser induced resonance fluorescence. Jour. Opt. Soc. Am. B32(9), 15751592.Google Scholar
Long, D. A. (2002). The Raman Effect: A Unified Treatment of the Theory of Raman Scattering by Molecules. John Wiley & Sons, Ltd.CrossRefGoogle Scholar
Siegman, A. E. (1986). Lasers. University Science Books.Google Scholar
She, C.-Y. (2001). Spectral structure of laser light scattering revisited: Bandwidths of non-resonant scattering lidars. Appl. Optics 40(27), 46754884.Google Scholar
Herzberg, G. (1950). Molecular Spectra and Molecular Structure: I. Spectra of Diatomic Molecules, 2nd ed. Van Nostrand Reinhold Company.Google Scholar
Foley, H. M. (1946). The pressure broadening of spectral lines. Phys. Rev. 69(1–12), 616628.CrossRefGoogle Scholar
Dicke, R. H. (1953). The effect of collisions upon the Doppler width of spectral lines. Phys. Rev. 89(2), 472473.Google Scholar
Galatry, L. (1961). Simultaneous effect of Doppler and foreign gas broadening on spectral lines. Phys. Rev. 122(4), 12181223, DOI: https://doi.org/10.1103/PhysRev.122.1218.Google Scholar
Rahn, L. A., and Palmer, R. E.. (1986). Studies of nitrogen self-broadening at high temperature with inverse Raman spectroscopy. JOSA-B, 3(9), 11641169.Google Scholar

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