Chemical composition of primary cosmic rays with energies from 1015 to 1016.5 eV

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dc.contributor.authorY. Shirasaki
dc.contributor.authorF. Kakimoto
dc.contributor.authorS. Ogio
dc.contributor.authorN. Gironda
dc.contributor.authorM. Takeda
dc.contributor.authorT. Kaneko
dc.contributor.authorH. Yoshii
dc.contributor.authorToshihiko Baba
dc.contributor.authorSakae Sano
dc.contributor.authorK. Nishi
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T15:41:37Z
dc.date.available2026-03-22T15:41:37Z
dc.date.issued2001
dc.descriptionCitaciones: 10
dc.identifier.doi10.1016/s0927-6505(00)00166-3
dc.identifier.urihttps://doi.org/10.1016/s0927-6505(00)00166-3
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/53857
dc.language.isoen
dc.publisherElsevier BV
dc.relation.ispartofAstroparticle Physics
dc.sourceTokyo Institute of Technology
dc.subjectCosmic ray
dc.subjectPhysics
dc.subjectPrimary (astronomy)
dc.subjectSupernova
dc.subjectAstrophysics
dc.subjectMonte Carlo method
dc.subjectStars
dc.subjectChemical composition
dc.subjectNuclear physics
dc.titleChemical composition of primary cosmic rays with energies from 1015 to 1016.5 eV
dc.typearticle

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