Abstract
The determinat ion of t r ansmiss ion functions on the basis of distinct model representa t ions is of great significance in the problem of t r ansmiss ion of infrared emiss ion through the a tmosphere . The s imples t model of a group of spec t ra l l ines is the E l sas se r model of equidistant lines of identical intensity. According to that model, the average absorpt ion A t in a given spectra l interval in the weak-l ine approximation (u << 1) is given by
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