A comparative analysis of gamma and hadron families at the superhigh energies recorded in experiment PAMIR

Details A comparative analysis of gamma and hadron families at the superhigh energies recorded in experiment PAMIR A comparative analysis of gamma and hadron families at the superhigh energies recorded in experiment PAMIR

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..424a&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 424-427 (SEE N85-35848 24-93)

Computer Science

Anisotropy, Azimuth, Bubble Chambers, Cascade Flow, Chemical Composition, Cosmic Ray Showers, Electromagnetic Radiation, Gamma Rays, Hadrons, High Energy Interactions, Models, Charged Particles, Collision Parameters, Nuclear Scattering

Scientific paper

A comparative analysis of hadron and gamma families which have undergone the decascading procedure is made. Results are compared with different models of interactions. In hadron families with energies Summary EHgamma 20 TeV as well as in gamma families with energies Summary Egamma 70 TeV, increasing azimuthal anisotropy is observed.

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