Abstract

We have measured the absolute vertical integral and differential cosmic-ray single-muon flux at 3.6 GeV. The apparatus consisted of two 100 in. high iron absorbers placed between large counter arrays. The iron absorbers could be magnetized with current-carrying coils wrapped around term. The differential flux was obtained from flux measurements at different magnetic-field values. Adjacent counters were used to correct the data for cosmic-ray showers and to provide parallel counter telescopes to look for penetrating pairs due to μ,’s or quarks. The measured integral flux at 3.6GeV was (1.83±0.4).10-3/cm2.sr.s, and the differential flux was (l.28±0.25).10-3cm-2.sr.GeV.s. The showerless μ-pair flux was measured to be (0.58.10-6±0.58.10-5)/cm2.sr.s for pairs between 0in. and 30 in. apart, and (1.68 -10-6 ±1.68. 10-5)/cm2.sr.s for pairs between 30 in. and 60 in.

Full Text
Paper version not known

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 call

Disclaimer: 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.