Jet phenomena in a giant superfamily

Details Jet phenomena in a giant superfamily Jet phenomena in a giant superfamily

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985izyak..49.1278b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Astronomy and Astrophysics

Astronomy

Electron Photon Cascades, Energetic Particles, Gamma Ray Astronomy, Nuclear Interactions, High Energy Interactions, Spatial Distribution, X Ray Analysis

Scientific paper

The total energy of the gamma component of the Fianit superfamily recorded at the Pamir station is 3.2 x 10 to the 16th eV. It is noted that this superfamily is the most energetic event yet recorded by an X-ray emulsion chamber. It is characterized by the presence of a large number of groups (clusters) having a transverse momentum that is, on the average, 10 times greater than that of ordinary gamma-quanta.

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