塔吉克斯坦大气尘埃的光学厚度

Robert S. Fraser
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引用次数: 16

摘要

在塔吉克斯坦进行的一次尘埃实验中,气溶胶尘埃的光学厚度是由卫星对反射阳光的测量得出的。该方法估计了在低光学厚度的日子里,同一地面区域发生尘埃的表面反射率。为了避免沙尘天气和晴空天气之间地表双向反射率的变化,在沙尘暴发生前8天获得太阳方向和观测方向之间几乎相同的几何形状。使用查找表来获得晴天的表面反射率,并使用另一组查找表来指定尘埃的光学深度。光学深度查找表利用米氏散射的代表性尺寸分布和折射率的粉尘气溶胶。在地球上许多地点观测到的粉尘气溶胶的大小分布和折射率的相似性证明了这种方法的合理性。给出了尘埃光学厚度图。
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Optical thickness of atmospheric dust over Tadzhikistan

The aerosol dust optical thickness during a dust experiment in Tadzhikistan is derived from satellite measurements of reflected sunlight. The method estimates the surface reflectance on days with low optical thickness for the same ground area where dust occurs. In order to avoid changes in the surface bidirectional reflectance between the dusty and clear days, nearly identical geometry between the solar and view directions is obtained eight days before a dust storm. Lookup tables are utilized to obtain the surface reflectance on the clear day, and another set of lookup are tables is used to assign an optical depth to the dust. The optical depth lookup tables utilize Mie scattering for a representative size distribution and index of refraction for the dust aerosol. The observed similarity of size distributions and indices of refraction for dust aerosols at many locations over the earth justify this method. A map of the dust optical thickness is given.

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