Speaker
Miguel Molero Gonzalez
(Institute of Astrophysics of the Canary Islands (ES))
Description
Analysis of anisotropy of the arrival directions of galactic positrons, electrons and protons has been performed with the Alpha Magnetic Spectrometer on the International Space Station. This measurement allows to differentiate between point-like and diffuse sources of cosmic rays for the understanding of the origin of high energy positrons. The AMS results of the dipole anisotropy are presented along with the discussion of the implications of these measurements.
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Author
Miguel Molero Gonzalez
(Institute of Astrophysics of the Canary Islands (ES))
Co-authors
Inaki Rodriguez Garcia
(CIEMAT - Centro de Investigaciones Energéticas Medioambientales y Tec. (ES))
Jorge Casaus
(CIEMAT - Centro de Investigaciones Energéticas Medioambientales y Tec. (ES))
Miguel Angel Velasco Frutos
(CIEMAT - Centro de Investigaciones Energéticas Medioambientales y Tec. (ES))
