DocumentCode
2674001
Title
Statistical considerations on the extinction error variance for the raman lidar inversion algorithm
Author
Rocadenbosch, Francesc ; Comerón, Adolfo ; Sicard, Michaël ; Reba, Mohd Nadzri Md
Author_Institution
Univ. Polytech. de Catalunya (UPC), Barcelona
fYear
2007
fDate
23-28 July 2007
Firstpage
2771
Lastpage
2774
Abstract
At the basis of the Raman lidar extinction inversion algorithm is the derivative of the logarithm of the ratio between the atmospheric nitrogen number density and the range-corrected Raman power return. While its computation is straightforward under ideal (noiseless) conditions, this is not the case under low signal-to-noise ratios, for which the observation noise may lead the logarithm to singular values. This work presents an analytical-statistical overview of the inversion problem and related error bars, tentative noise limiting criteria, and justifies the approximations at play to estimate the inversion error by means of error-propagation techniques for high signal- to-noise ratios. Simulation examples consider a 532/607-nm elastic-Raman system.
Keywords
Raman spectra; atmospheric composition; atmospheric techniques; inverse problems; optical radar; remote sensing by laser beam; statistical analysis; Raman lidar inversion algorithm; analytical-statistical overview; atmospheric nitrogen number density; error bars; error propagation; extinction error variance; observation noise; range-corrected Raman power return; signal-to-noise ratio; tentative noise limiting criteria; Aerosols; Backscatter; Extinction coefficients; Gaussian noise; Laser radar; Nitrogen; Noise level; Optical scattering; Remote sensing; Signal to noise ratio; Lidar; Raman inversion; errorbars; extinction; logtransformed noise;
fLanguage
English
Publisher
ieee
Conference_Titel
Geoscience and Remote Sensing Symposium, 2007. IGARSS 2007. IEEE International
Conference_Location
Barcelona
Print_ISBN
978-1-4244-1211-2
Electronic_ISBN
978-1-4244-1212-9
Type
conf
DOI
10.1109/IGARSS.2007.4423417
Filename
4423417
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