Cosmic-ray family phenomenology of visible energy greater than 500 TeV observed in high mountain emulsion chambers

Details Cosmic-ray family phenomenology of visible energy greater than 500 TeV observed in high mountain emulsion chambers Cosmic-ray family phenomenology of visible energy greater than 500 TeV observed in high mountain emulsion chambers

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aipc..276...42h&link_type=abstract

The seventh international symposium on very high energy cosmic-ray interactions. AIP Conference Proceedings, Volume 276, pp. 42

Physics

Hadron-Induced High- And Super-High-Energy Interactions, Cosmic Rays

Scientific paper

The characteristics of hadron interactions are studied by surveying the family configurations on the event-based way for 75 cosmic-ray families of the highest energy range observed at Chacaltaya chambers and Pamir-joint chambers in total ~1,400 m2 yr exposure and the exotic type interactions ``Centauro-species'' are discussed from the point of view of family phenomenology.

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