AMS-gamma: high energy photons detection with the Alpha Magnetic Spectrometer on the ISS

Details AMS-gamma: high energy photons detection with the Alpha Magnetic Spectrometer on the ISS AMS-gamma: high energy photons detection with the Alpha Magnetic Spectrometer on the ISS

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....7.2777b&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

AMS is a large acceptance, superconducting magnetic spectrometer designed to study, with high accuracy, the composition of cosmic rays. We discuss how AMS will also identify γ rays in the energy interval 1-300 GeV , operating as a e+ e- pair spectrometer. During the scheduled threeyear mission on the International Space Station (ISS) starting in 2004, AMS will provide access to the largely unexplored γ energy range above 20 GeV complementary to other space missions and ground based Čherenkov detectors.

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