Speaker
Francesco Nozzoli
(TIFP)
Description
The fluxes and flux ratios of charged elementary particles in cosmic rays are presented in the absolute rigidity range from 1 to 1000 GV.
In the absolute rigidity range ∼60 to ∼500 GV, the antiproton, proton, and positron fluxes are found to have nearly identical rigidity dependence and the electron flux
exhibits different rigidity dependence. Below 60 GV, the antiproton-to-proton, antiproton-to-positron, and proton-to-positron flux ratios each reaches a maximum.
Particular emphasis is made on new observations of the properties of elementary particles in the rigidity range above 500 GV.
Primary author
Francesco Nozzoli
(TIFP)
