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The atmospheric radiation correction plays an important role in the preprocessing of remote sensing images. After a long period of researching and developing, there are some well- developed packages, such as LOWTRAN 7 and 5S, which are good in calculating the atmospheric transmittance. In general, some packages require the input parameters, like visibility, asymme- try factor, phase function, ozone content...etc., but they can' t be acquired quantitatively by users. For this reason, the precision of the computed atmospheric transmittance is often poor. The purpose of this research is to estimate the visibility quantitatively. Aerosol extinction, Rayleigh extinction and gases absorption cause the main variation of the atmospheric transmittance. But only the aerosol extinction is related to the variation of visibility. In order to estimate the visibility, those effects that are indifferent of the variation of visibility must be eliminated from the calculation of atmospheric transmittance. By using some wide-band models to do so, the visibility can be estimated from the aerosol extinction. Thereafter, accompanied with the observed visibility, one can compare it with the theoretical results to diagnose the characteristics of individual models. The precision of using visibility to describe the detail of aerosol is limitted. Nevertheless, as the input parameter for the packages mentioned above, the estimated visibility in this study is reliable and acceptable.
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