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

机译:利用宽带太阳掩星技术检索温度和压力:SOFIE方法和结果

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Measurement of atmospheric temperature as a function of pressure, T(P), 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 T(P) using both broadband transmittance and refraction are discussed. Investigations using measurements of broadband transmittance in two CO2 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.
机译:大气温度随压力的变化 T(P)是理解许多大气过程的关键,也是从太阳掩星测量中获取气体混合比和其他参数的前提。本文简要概述了太阳掩星测量技术,然后详细讨论了使测量对温度敏感的机制。讨论了利用宽带透射率和折射来检索 T(P)的方法。然后介绍了使用两个CO 2 吸收带(4.3和2.7μm频带)和折射弯曲的宽带透射率测量进行的研究。这些调查包括敏感性研究,模拟检索研究以及来自SOFIE的示例。

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