Atmospheric Muon Charge Ratio Analysis at the INO-ICAL Detector

Figure 9

Muon flux generated using CORSIKA at the top of the hill (i.e. 2 k.m. above the sea level) with primary protons in energy range 1-20 TeV(brown dots) and its comparison with the existing experimental fluxes ( [2],[7], +[8], [9], [10]) and the flux (solid blue line) from [11].