Energetic delayed hadrons in large air showers observed at 5200m above sea level

dc.contributor.authorT. Kaneko
dc.contributor.authorK. Hagiwara
dc.contributor.authorH. Yoshii
dc.contributor.authorN. Martinić
dc.contributor.authorL. Siles
dc.contributor.authorP. Miranda
dc.contributor.authorF. Kakimoto
dc.contributor.authorI. Tsuchimoto
dc.contributor.authorN. Inoue
dc.contributor.authorK. Suga
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T17:00:48Z
dc.date.available2026-03-22T17:00:48Z
dc.date.issued1985
dc.description.abstractEnergetic delayed hadrons in air showers with electron sizes in the range 10 to the 6th power to 10 to the 9th power were studied by observing the delayed bursts produced in the shield of nine square meter scintillation detectors in the Chacaltaya air-shower array. The frequency of such delayed burst is presented as a function of electron size, core distance and sec theta.
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/61647
dc.language.isoen
dc.sourceOkayama University
dc.subjectPhysics
dc.subjectNuclear physics
dc.subjectHadron
dc.subjectRange (aeronautics)
dc.subjectAir shower
dc.subjectElectron
dc.subjectScintillation
dc.subjectAstrophysics
dc.subjectEnvironmental science
dc.subjectCosmic ray
dc.titleEnergetic delayed hadrons in large air showers observed at 5200m above sea level
dc.typearticle

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