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[en] The spectra of cosmic pions and kaons produced at the top the atmosphere have been derived from the primary cosmic ray spectrum of Grigorov et al. by using the Bose-type model. With the help of pion and kaon atmospheric diffusion equations the muon spectra at different atmospheric depths viz., 690, 535 and 1033 g cm-2 have been estimated. The results are in accord with the magnetic spectrograph data of Kocharian et al. and Allkofer et al. (author)
Journal
Annalen der Physik (Leipzig); ISSN 0003-3804; 
; v. 36(1); p. 47-51
; v. 36(1); p. 47-51