Problem of Coplanarity of Energy Flows in EAS Cores
摘要
The effect of the trend that, according to observations in high-altitude and stratospheric experiments with x-ray emulsion chambers, the most energetic particles and/or groups of particles in gamma–hadron families show toward coplanar arrival is discussed. Experimental data are compared with the results of calculations performed within various versions of the FANSY 2.0 model, which include a version that reproduces coplanar generation of the most energetic particles in hadron interactions at ultrahigh energies. The whole body of experimental data on azimuthal characteristics of gamma–hadron families observed at the levels of 25, 75, and 600 g/cm