EPJ Web Conf.
Volume 209, 2019RICAP18, 7th Roma International Conference on Astroparticle Physics
|Number of page(s)||4|
|Published online||13 May 2019|
Properties of Elementary Particle Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station
INFN TIFPA, I-38123 Trento, Italy
a e-mail: Francesco.Nozzoli@tifpa.infn.it
Published online: 13 May 2019
Precision measurements by AMS of the fluxes of cosmic ray positrons, electrons, antiprotons, protons as well as their rations reveal several unexpected and intriguing features. The presented measurements extend the energy range of the previous observations with much increased precision. The new results show that the behavior of positron flux at around 300 GeV is consistent with a new source that produce equal amount of high energy electrons and positrons. In addition, in the absolute rigidity range 60–500 GV, the antiproton, proton, and positron fluxes are found to have nearly identical rigidity dependence and the electron flux exhibits different rigidity dependence.
© The Authors, published by EDP Sciences, 2019
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