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VOLUME 56 (1992) | ISSUE 4 | PAGE 192
Alignment in gamma-hadron families of cosmic rays and interaction characteristics at E_0\sim 10^{16} eV
An alignment of the basic energy fluxes in families of cosmic-ray particles along a straight line has been observed. This effect depends on the interaction energy. It is evident that the separation of the secondary particles in nuclear-interaction events at heights not far above the apparatus is coplanar at ultrahigh energies {E0> 1016 eV).