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Satellite Measurement of Stratospheric Winds and Ozone Using Doppler Michelson Interferometry. Part Ⅰ: Instrument Model and Measurement Simulation

机译:使用多普勒·迈克尔逊干涉仪对平流层风和臭氧进行卫星测量。第一部分:仪器模型与测量仿真

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This paper presents an instrument model and observation simulations for the measurement of stratospheric winds and ozone concentration using a satellite instrument employing imaging and the Doppler Michelson interferometery technique. The measurement technique and instrument concept are described. The instrument model and simulations are based on initial design characteristics of the Canadian Stratospheric Wind Interferometer for Transport Studies (SWIFT) satellite instrument. SWIFT employs an imaging array and a field-widened Michelson interferometer. It will measure stratospheric winds and ozone densities using the wind-induced phase shifts of interferograms from atmospheric limb radiance spectra in the vicinity of the vibration-rotation ozone line at 1133.4335 cm~(-1). The measurement simulation and analysis tools have been developed to assess the SWIFT instrument performance and to evaluate the impact of instrument and measurement characteristics on expected wind and ozone errors. Sample results of the measurement simulation and the related line-of-sight wind error noise levels are presented.
机译:本文介绍了使用卫星成像仪和多普勒·迈克尔逊干涉仪技术测量平流层风和臭氧浓度的仪器模型和观测模拟。描述了测量技术和仪器概念。仪器模型和仿真基于加拿大用于运输研究的平流层风干涉仪(SWIFT)卫星仪器的初始设计特征。 SWIFT采用了成像阵列和加宽的迈克尔逊干涉仪。它将利用来自1133.4335 cm〜(-1)振动旋转臭氧线附近大气肢体辐射光谱的干涉图的风致相移来测量平流层风和臭氧密度。已经开发出了测量模拟和分析工具,以评估SWIFT仪器的性能,并评估仪器和测量特性对预期的风和臭氧误差的影响。给出了测量模拟的示例结果以及相关的视线风误差噪声级。

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