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Optical Properties of the Undisturbed Mesosphere from Wide-Angle Twilight Sky Polarimetry

机译:广角暮光天空偏振法对未扰动中球的光学性质

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The paper describes the first results of all-sky polarization measurements of the twilight background started in central Russia in the very beginning of summer 2011. Time-frequency data of the sky intensity and polarization over a wide range of sky point zenith distances are used to separate single and multiple scattering and construct the altitude dependence of the scattering coefficient and polarization in the mesosphere (altitudes from 60 to 90 km) at different angles. The undisturbed structure of the mesosphere without noticeable aerosol stratification on observation days makes it possible to estimate the temperature of the atmosphere at these altitudes.
机译:本文介绍了从2011年夏季开始在俄罗斯中部开始的暮光背景全天空极化测量的最初结果。使用了在广泛的天空点天顶距离范围内的天空强度和极化的时频数据,分离单次和多次散射,并构造不同角度的中层(60至90 km高度)散射系数和极化的高度相关性。在观测日没有明显的气溶胶分层的中层结构不受干扰,可以估算出这些海拔高度的大气温度。

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