Speaker
Stanislav Knurenko
Description
The article considers showers produced by primary particles with energies E0 ≥ 100 EeV. The showers were registered in the course of continuous long-term observations at the Yakutsk array of extensive air showers. In the present work, the mathematical processing of showers was repeated and the phenomenology of the charged component, muons with threshold thr, 1 GeV and radio emission in the region of highest energies was refined. The characteristics of cosmic rays are analyzed: the energy spectrum and mass composition determined from the Cherenkov, muon components and radio emission in the energy range 50 – 200 EeV.
Primary authors
Stanislav Knurenko
Igor Petrov
(Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy)
