Speaker
Miguel Molero Gonzalez
(Centro de Investigaciones Energéti cas Medioambientales y Tecno)
Description
Analysis of anisotropy of the arrival directions of galactic protons, electrons and positrons has been performed with the Alpha Magnetic Spectrometer on the International Space Station. These results allow to differentiate between point-like and diffuse sources of cosmic rays for the explanation of the observed excess of high energy positrons. The AMS results on the dipole anisotropy are presented along with the discussion of implications of these measurements.
Authors
Miguel Molero Gonzalez
(Centro de Investigaciones Energéti cas Medioambientales y Tecno)
Giuseppe La Vacca
(Universita & INFN, Milano-Bicocca (IT))
Jorge Casaus
(Centro de Investigaciones Energéti cas Medioambientales y Tecno)
Iris Gebauer
(KIT - Karlsruhe Institute of Technology (DE))
