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In this work is obtained new approximation for the yield function Y forcosmic ray induced ionization in the Earth atmosphere on the basis of simulateddata. The parameterization is obtained using inverse nonlinear problem solutionwith afxy(analyze fx=y)-code. Short description of the methods is given. Thefound approximation is for primary proton nuclei, inclined up to 70 degreeszenith angle. This permits to estimate the direct ionization by primary cosmicrays explicitly. The parameterization is applicable to the entire atmosphere,from ground level to upper atmosphere. Several implications of the foundparameterization are discussed.

Application of afxy-code for parameterization of ionization yield function Y in the atmosphere for primary cosmic ray protons