Muon time spread in EAS, 10 to the 17th - 10 to the 18th eV

Details Muon time spread in EAS, 10 to the 17th - 10 to the 18th eV Muon time spread in EAS, 10 to the 17th - 10 to the 18th eV

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....6..129b&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 6 (A85-2

Physics

Cosmic Ray Showers, Muons, Radiation Measurement, Cerenkov Radiation, Particle Energy, Scintillation Counters, Time Response

Scientific paper

The pulse rise times from 10 to 70 percent of full amplitude (T70) of the response of three 10-sq-m liquid scintillators in the infilled section of the water Cerenkov detector array at Haverah Park to EAS muons are determined experimentally with accuracy about 1 nsec. The vertical muon threshold energies of the detectors are given as 420, 489, and 318 MeV, with a density dynamic range of 15-100 muons/10 sq m. Five pulse types are observed; the variation of T70 with EAS core distance and zenith angle is plotted for types 1 and 2 and analyzed statistically; and the type 3, 4, and 5 profiles are characterized. The mean T70 values from the statistical analysis are found to be in agreement with those of Blake et al. (1982) but significantly faster than those predicted by theoretical models, even with Fe primaries.

Affiliated with

Also associated with

No associations

Rating

Muon time spread in EAS, 10 to the 17th - 10 to the 18th eV does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Muon time spread in EAS, 10 to the 17th - 10 to the 18th eV, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Muon time spread in EAS, 10 to the 17th - 10 to the 18th eV will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-745517