Skip to main content Accessibility help
×
Hostname: page-component-76fb5796d-2lccl Total loading time: 0 Render date: 2024-04-27T20:51:05.249Z Has data issue: false hasContentIssue false

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
Get access

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

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

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

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×