Results on high-energy cosmic rays by EAS-TOP at Gran Sasso.

Details Results on high-energy cosmic rays by EAS-TOP at Gran Sasso. Results on high-energy cosmic rays by EAS-TOP at Gran Sasso.

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ncimc..20..985a&link_type=abstract

Nuovo Cimento C, Vol. 20C, N. 6, p. 985 - 1007

Computer Science

Performance

Air Showers: Detectors

Scientific paper

Very high-energy cosmic rays have to be studied through the ground-based detectors of the extensive air showers (EAS) that they produce in the atmosphere. The main measurements to be performed are of: primary energy spectra, composition, anisotropies, "neutral primary" astronomy, and interaction properties. This requires complete detectors of all the EAS components, and for this purpose the EAS-TOP array has been constructed at Campo Imperatore (2000 m a.s.l.) on top of the Gran Sasso underground laboratories. The array has been progressively going into operation since 1988. The authors present the status and performances of the different detectors, and the results obtained up to now on the different items under discussion.

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