Abstract
For pt.I see ibid., vol.3, p.979 (1977). The expected cosmic-ray burst spectrum ( approximately 1 TeV) in a lead target at sea level has been determined using the published hadronic and muonic spectra. The response of the recording scintillator detector is carefully assessed. The muon burst size spectrum is straightforwardly calculated. Two different approaches are used to determine the expected hadronic burst spectrum, one an analytical technique and the other a Monte-Carlo method. Good agreement between the two techniques is found. The Monte-Carlo method has the advantage of taking into account multiple hadron interactions. The results are compared with experimental data derived from the scintillator detector. The muon-initiated burst spectrum shows close agreement, but a discrepancy of at least a factor of three appears between calculated and measured intensities of hadron-induced bursts.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
