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Muon Spectra at Different Altitudes Derived from Bose‐Type Model
Author(s) -
Ghosh A. K.,
Das N. C.,
Khalil Md.,
Bhattacharyya D. P.
Publication year - 1979
Publication title -
annalen der physik
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.009
H-Index - 68
eISSN - 1521-3889
pISSN - 0003-3804
DOI - 10.1002/andp.19794910108
Subject(s) - physics , pion , spectral line , muon , spectrograph , cosmic ray , atmosphere (unit) , nuclear physics , cosmic cancer database , spectrum (functional analysis) , particle physics , astrophysics , meteorology , quantum mechanics
The spectra of cosmic pions and kaons produced at the top of 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 K OCHARIAN et al. and A LLKOFER et al.