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Spectral and Spatial Dependency of Aerosol Extinction in the Upper Troposphere Based on the Moon Surface Photometry in the Earth's Umbra

机译:基于地球本影上月球表面光度法的对流层上层气溶胶消光的光谱和空间依赖性

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The work is based on photometry of the Moon's surface during the total lunar eclipse of June 15, 2011. Photometric data are used to retrieve the value of aerosol extinction coefficient in the troposphere above the Earth's limb in various spectral bands in the optical and near-I R ranges. The results are analyzed in comparison with the data of previous eclipses in 2004-2008. The main result consists in an increased aerosol concentration in the South-East Asia, which is maximum among all eclipses observed in recent years. At the same time, no relationship between eclipse brightness and solar activity is observed, as well as unified latitude dependency of umbra brightness noticed earlier.
机译:该工作基于2011年6月15日整个月蚀期间月球表面的光度学。光度学数据用于检索光学和近距离中各个光谱带中地球上肢对流层中气溶胶的消光系数值。 I R范围。将结果与2004-2008年以前的日食数据进行了比较。主要结果是东南亚的气溶胶浓度增加,这是近年来观察到的所有日食中最高的。同时,没有观测到日食亮度与太阳活动之间的关系,也没有观察到之前提到的本影亮度的统一纬度依赖性。

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  • 来源
    《Cosmic research》 |2012年第5期|p.340-345|共6页
  • 作者单位

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya ul. 84/32, Moscow 117997, Russia;

    Space Research Institute, Russian Academy of Sciences, Profsoyuznaya ul. 84/32, Moscow 117997, Russia,Moscow State University, Sternberg Astronomical Institute, Universitetskii prosp. 13, Moscow 119992, Russia;

    "Ka-Dar" Scientific Center, 1st Neopalimovskiiper. 16/13, Moscow 119121, Russia;

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