Identification of light and very heavy cosmic ray primaries at E0 ≍ 1015eV from surface and deep underground measurements at the Gran Sasso Laboratories.

Details Identification of light and very heavy cosmic ray primaries at E0 ≍ 1015eV from surface and deep underground measurements at the Gran Sasso Laboratories. Identification of light and very heavy cosmic ray primaries at E0 ≍ 1015eV from surface and deep underground measurements at the Gran Sasso Laboratories.

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999nuphs..70..512n&link_type=abstract

Nuclear Physics B - Proceedings Supplements, vol. 70, issue 1-3, pp. 512-514

Physics

Nuclear Physics

Cosmic Rays: Detection, Cosmic Rays: Detectors

Scientific paper

'Very heavy' (iron-like) and 'light' (proton-like) cosmic ray primaries
are identified at primary energies E0 ≍
1015eV by means of simultaneous measurements of shower size
at the Gran Sasso Laboratories by EAS-TOP and LVD deep underground.

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