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首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Understanding uncertainties in the retrieval of polar mesospheric clouds from the cloud imaging and particle size experiment in the presence of a bright Rayleigh background
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Understanding uncertainties in the retrieval of polar mesospheric clouds from the cloud imaging and particle size experiment in the presence of a bright Rayleigh background

机译:在存在明亮瑞利背景的情况下,通过云成像和粒径实验了解极性中层云的反演中的不确定性

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摘要

This paper presents a framework for understanding and quantifying the leverage available for inverting the radiance signal in order to retrieve particle size distribution mode radius and albedo from polar mesospheric clouds (PMC) observations using the cloud imaging and particle size (CIPS) instrument on board the aeronomy of ice in the mesosphere (AIM) satellite. The observed signal is a superposition of the scattering angle dependence of the cloud albedo and the Rayleigh scattered albedo controlled by ozone at the stratopause. The leverage as is defined in the paper is a way to quantify how much the net scattering angle dependence changes as a function of mode radius. The leverage is determined by decomposing the observed signal into orthogonal components which isolate the parts of the signal that are unique to changes in mode radius from those that could be due to changes in the background. This leverage is considered along with instrument noise performance to determine retrieval uncertainties and to understand minimum thresholds in the cloud retrieval parameters.
机译:本文提出了一个框架,该框架用于理解和量化可用于反转辐射信号的杠杆率,以便使用机载云成像和粒度(CIPS)仪器从极地中层云(PMC)观测中检索粒度分布模式半径和反照率。中层(AIM)卫星中的冰的天文学。观测到的信号是层状顶上由臭氧控制的云反照率和瑞利散射反照率的散射角依赖性的叠加。本文中定义的杠杆作用是一种量化净散射角依赖性随模半径变化的方式。通过将观察到的信号分解为正交分量来确定杠杆,正交分量将正交于模式半径变化的信号部分与可能由于背景变化而引起的信号部分隔离开来。该杠杆作用与仪器噪声性能一起考虑,以确定恢复不确定性并了解云恢复参数中的最小阈值。

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