Article ID Journal Published Year Pages File Type
10704045 Journal of Atmospheric and Solar-Terrestrial Physics 2005 5 Pages PDF
Abstract
The Raman backscatter cross sections for a 355 nm light source for the three fine-structure components are calculated. The signal-to-noise considerations show that the determination of the densities of the three fine-structure components separately is a feasible experiment. Since these fine-structure components are calculated to be in local thermodynamic equilibrium up to at least 350 km altitude, this experiment also gives atmospheric temperature. It is pointed out that this experiment does not suffer from the drawbacks of the previous efforts to determine atomic oxygen density and should yield reliable results for this density as well as temperature.
Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Geophysics
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