首页> 外文会议>Conference on Sensors, Systems, and Next-Generation Satellites VII; Sep 8-10, 2003; Barcelona, Spain >Data Retrieval and Error Analysis Study on the Measurement of Stratospheric Winds with a Michelson Interferometer
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Data Retrieval and Error Analysis Study on the Measurement of Stratospheric Winds with a Michelson Interferometer

机译:用迈克尔逊干涉仪测量平流层风的数据检索和误差分析研究

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The Stratospheric Wind Interferometer for Transport studies (SWIFT) instrument is designed to measure stratospheric winds in the altitude region of 20-45 km with a target accuracy of 3-5 m s~(-1). It is one of two scientific instruments on the Greenhouse Gases Observations Satellite (GOSAT) proposed for launch in 2008. The winds are to be determined by measuring the Doppler shift of thermal emission lines in a narrow spectral range using a limb viewing field widened Michelson interferometer. The instrument spectral range for this study is centered about a reference ozone line at 1133.4335 cm~(-1) with a full-width at half-maximum of ~0.1 cm~(-1) for the instrument transmittance function. Measurement simulation and data retrieval are applied in the present investigation to evaluate and elaborate on measurement and processing conditions required to satisfy the desired wind accuracy. The related principles, processes, and tools are summarized. Radiative transfer and instrumental measurement simulations are conducted to produce raw image measurements. These raw images are processed up to and including inversions performed using the maximum a posteriori solution equation with differential regularization. In addition to retrieving the Doppler wind and ozone number density profiles, allowance is made to investigate the additional recovery of parameters such a pressure scaling factor and profiles of temperature and nitrous oxide. Retrieval characterization and an error analysis have been undertaken. Introductory results are presented. Retrieval Doppler wind noise levels of under 3 m s~(-1) are obtained.
机译:运输用平流层风干涉仪(SWIFT)仪器旨在测量20-45 km海拔区域内的平流层风,目标精度为3-5 m s〜(-1)。它是拟于2008年发射的温室气体观测卫星(GOSAT)上的两种科学仪器之一。通过使用四角视场加宽的迈克尔逊干涉仪在狭窄的光谱范围内测量热辐射线的多普勒频移来确定风向。 。本研究的仪器光谱范围以参考臭氧线为中心,在1133.4335 cm〜(-1)处,半峰宽为〜0.1 cm〜(-1),代表仪器的透射率。在本研究中,将测量模拟和数据检索应用于评估和阐述满足期望的风速精度所需的测量和处理条件。总结了相关的原理,过程和工具。进行辐射传输和仪器测量模拟以产生原始图像测量值。这些原始图像最多可以处理并包括使用带有差分正则化的最大后验解方程执行的反演。除了获取多普勒风和臭氧数量密度分布图之外,还可以研究其他恢复参数的方法,例如压力定标因子以及温度和一氧化二氮的分布图。检索特性和错误分析已经进行。介绍了介绍结果。获得的多普勒风噪声水平低于3 m s〜(-1)。

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