“…Long-duration balloon experiments like ATIC [1], TRACER [2], CREAM [3] allowed to determine fine structure of cosmic rays spectra up to 10 14 eV. With huge interest new data on protons, nuclei and electrons spectra obtained by space experiments PAMELA [4], AMS02 [5], ATIC [6], FermiLAT [7], NUCLEON [8], CALET [9], DAMPE [10] was accepted and interpreted. Above-mentioned experiments won't be able to solve completely these tasks.…”