NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Longitudinal development of muons in large air showers studies from the arrival time distributions measured at 900m above sea levelThe arrival time distributions of muons with energies above 1.0GeV and 0.5GeV have been measured in the Akeno air-shower array to study the longitudinal development of muons in air showers with primary energies in the range 10 to the 17th power to 10 to the 18th power ev. The average rise times of muons with energies above 1.0GeV at large core distances are consistent with those expected from very high multiplicity models and, on the contrary, with those expected from the low multiplicity models at small core distances. This implies that the longitudinal development at atmospheric depth smaller than 500 cm square is very fast and that at larger atmospheric depths is rather slow.
Document ID
19850027742
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Kakimoto, F.
(Tokyo Inst. of Tech. Tokyo, Japan)
Tsuchimoto, I.
(Tokyo Inst. of Tech. Tokyo, Japan)
Enoki, T.
(Tokyo Inst. of Tech. Tokyo, Japan)
Suga, K.
(Tokyo Inst. of Tech. Tokyo, Japan)
Nishi, K.
(Inst. of Physical and Chemical Research)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 7
Subject Category
Space Radiation
Report/Patent Number
HE-4.7-4
Accession Number
85N36055
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
No Preview Available