Observational Characteristics of MAS Array at Mt. Chacaltaya.

Details Observational Characteristics of MAS Array at Mt. Chacaltaya. Observational Characteristics of MAS Array at Mt. Chacaltaya.

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....3..239y&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

Observations of energy spectrum and chemical composition in primary cosmic rays near "Knee" with sufficient statistics give important information to study sources and propagation of cosmic rays in the galaxy. As the statistics is not sufficient in direct measurements on balloon-borne experiments, so observations of air showers at high mountain site are necessary to increase the statistics of events in the energy region. We have rearranged MAS array for observations of observable minimum air shower at Mt. Chacaltaya (5200m a.s.l.) for those purposes. So, characteristics of MAS array in observation of air showers with energies above the threshold energy 6TeV (triggering efficiency 50%) and preliminary results will be reported.

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