Fractions of proton, helium, middle and heavy nuclei in primary cosmic rays at energy 10**16eV

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dc.creatorKalmakhelidze, Maia
dc.creatorRoinishvili, Nina
dc.creatorSvanidze, Manana
dc.date2001-07-06
dc.date.accessioned2026-07-07T03:34:40Z
dc.date.available2026-07-07T03:34:40Z
dc.descriptionClassification of gamma-hadron families, registered by the Pamir collaboration, on four groups of nuclei (P, He, middle and heavy), responsible for their generation, is made, and fractions of families in each of the groups are estimated. Results show, that below the knee of the energy spectrum the chemical composition of primary cosmic rays remains close to the normal one.
dc.description6 pages (REVTeX), 1 eps figure, Published in the Proceeding of 26th Russian Conference on Cosmic Rays (Izv. RAN ser.Fiz.)
dc.identifierhttps://arxiv.org/abs/hep-ex/0107011
dc.identifierhttp://arxiv.org/abs/hep-ex/0107011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/37068
dc.subjectHigh Energy Physics - Experiment
dc.titleFractions of proton, helium, middle and heavy nuclei in primary cosmic rays at energy 10**16eV
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