Monostatic propagation channel enhanced backscatter effects: a comparison of refractive spectral models

Details Monostatic propagation channel enhanced backscatter effects: a comparison of refractive spectral models Monostatic propagation channel enhanced backscatter effects: a comparison of refractive spectral models

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996spie.2828..178a&link_type=abstract

Proc. SPIE Vol. 2828, p. 178-188, Image Propagation through the Atmosphere, J. C. Dainty; Luc R. Bissonnette; Eds.

Physics

Scientific paper

Enhanced backscatter effects associated with the mean intensity and scintillation index for a monostatic propagation channel through atmospheric turbulence are analyzed for two spectral models of refractive-index fluctuations. The analysis presented here shows that using a more physically realistic modified spectrum with inner and outer scale parameters as well as a high-wave-number rise (bump) can lead to significantly different results than those predicted by the idealized Kolmogorov power law spectrum. The target models used in this analysis include a smooth target finite mirror, glint target finite retroreflector, and a rough surface target (Lambert surface). The general method of analysis is based on weak fluctuation theory.

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