Penetrative nature of high energy showers observed in Chacaltaya emulsion chamber

Details Penetrative nature of high energy showers observed in Chacaltaya emulsion chamber Penetrative nature of high energy showers observed in Chacaltaya emulsion chamber

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..284f&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 284-287 (SEE N85-35848 24-93)

Other

Cosmic Ray Showers, Electromagnetic Scattering, Hadrons, High Energy Interactions, Mean Free Path, Clumps, Collision Parameters, Particle Collisions, Pattern Recognition

Scientific paper

About 30% of single core showers with E gamma 10 TeV have stronger penetrating power than that expected from electromagnetic showers (e,gamma). On the other hand, their starting points of cascades in the chamber are found to be as shallow as those of (e,gamma) components. It is suggested that those showers are very collimated bundles of hadron and (e,gamma) component. Otherwise, it is assumed that the collision mean free path of those showers in the chamber is shorter than that of hadron with geometrical value.

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