Retrieval of temperature and pressure using broadband solar occultation: SOFIE approach and results

Measurement of atmospheric temperature as a function of pressure, <i>T(P)</i>, is key to understanding many atmospheric processes and a prerequisite for retrieving gas mixing ratios and other parameters from solar occultation measurements. This paper gives a brief over...

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Bibliographic Details
Main Authors: B. T. Marshall, L. E. Deaver, R. E. Thompson, L. L. Gordley, M. J. McHugh, M. E. Hervig, J. M. Russell III
Format: Article
Language:English
Published: Copernicus Publications 2011-05-01
Series:Atmospheric Measurement Techniques
Online Access:http://www.atmos-meas-tech.net/4/893/2011/amt-4-893-2011.pdf
Description
Summary:Measurement of atmospheric temperature as a function of pressure, <i>T(P)</i>, is key to understanding many atmospheric processes and a prerequisite for retrieving gas mixing ratios and other parameters from solar occultation measurements. This paper gives a brief overview of the solar occultation measurement technique followed by a detailed discussion of the mechanisms that make the measurement sensitive to temperature. Methods for retrieving <i>T(P)</i> using both broadband transmittance and refraction are discussed. Investigations using measurements of broadband transmittance in two CO<sub>2</sub> absorption bands (the 4.3 and 2.7 μm bands) and refractive bending are then presented. These investigations include sensitivity studies, simulated retrieval studies, and examples from SOFIE.
ISSN:1867-1381
1867-8548