Characteristics of EAS and Primary Particle Mass Composition in the Energy Region of $10^{17} - 3 \cdot 10^{19}$ eV by Yakutsk Data

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dc.creatorKnurenko, S. P.
dc.creatorEgorova, V. P.
dc.creatorIvanov, A. A.
dc.creatorKolosov, V. A.
dc.creatorMakarov, I. T.
dc.creatorPetrov, Z. E.
dc.creatorSleptsov, I. Ye.
dc.creatorStruchkov, G. G.
dc.date2004-11-17
dc.date.accessioned2026-07-07T02:15:53Z
dc.date.available2026-07-07T02:15:53Z
dc.descriptionIn the work the data of the Yakutsk complex EAS array and their comparison with calculation in the case of primary nuclei of different chemical elements are presented. The calculation by QGSJET model have been used interpreting experimental data.
dc.descriptionXIII International Symposium on Very High Energy Cosmic Ray Interaction, Pylos Greece, 6 - 12 Sep 2004. Four pages, three figures. Submitted for publication in Nuclear Physics (B)
dc.identifierhttps://arxiv.org/abs/astro-ph/0411483
dc.identifierhttp://arxiv.org/abs/astro-ph/0411483
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8583
dc.subjectAstrophysics
dc.titleCharacteristics of EAS and Primary Particle Mass Composition in the Energy Region of $10^{17} - 3 \cdot 10^{19}$ eV by Yakutsk Data
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