Arrival-time distribution of muons and electrons in large air showers observed at 5200m above sea level

Simple item page
dc.contributor.authorC. Aguirre
dc.contributor.authorR. Anda
dc.contributor.authorA. Trepp
dc.contributor.authorF. Kakimoto
dc.contributor.authorY. Mizumoto
dc.contributor.authorK. Suga
dc.contributor.authorN. Izu
dc.contributor.authorY. Kamouchi
dc.contributor.authorN. Inoue
dc.contributor.authorShinsuke Kawai
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T17:37:56Z
dc.date.available2026-03-22T17:37:56Z
dc.date.issued1979
dc.description.abstractAn experiment is going on at Mt. Chacaltaya in Bolivia (550 gcm−2 atmospheric depth) to observe arrival‐time distributions of muons and electrons in air showers above 1017 eV to study the early stage of longitudinal development related directly with the character of nuclear interactions and the composition of primary cosmic rays at these high energies. The preliminary results are presented at the Seminar.
dc.identifier.doi10.1063/1.31608
dc.identifier.urihttps://doi.org/10.1063/1.31608
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/65324
dc.language.isoen
dc.publisherAmerican Institute of Physics
dc.relation.ispartofAIP conference proceedings
dc.sourceHigher University of San Andrés
dc.subjectElectron
dc.subjectMuon
dc.subjectPhysics
dc.subjectDistribution (mathematics)
dc.subjectEnvironmental science
dc.subjectArrival time
dc.subjectNuclear physics
dc.subjectAtmospheric sciences
dc.titleArrival-time distribution of muons and electrons in large air showers observed at 5200m above sea level
dc.typearticle

Files

Collections

Artículo Científico Publicado