Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..235e&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 235-238 (SEE N85-35968 24-93)
Astronomy and Astrophysics
Astronomy
Background Radiation, Cosmic Ray Showers, Gamma Rays, Hadrons, Muons, Particle Collisions, Anisotropy, Detection, Gamma Ray Astronomy, Models
Scientific paper
The result of a calculation of the expected number of muons in gamma ray initiated and cosmic ray initiated air showers using a realistic model of hadronic collisions in an effort to understand the available experimental results and to assess the feasibility of using the muon content of showers as a veto to reject cosmic ray initiated showers in ultra-high energy gamma ray astronomy are reported. The possibility of observing very-high energy gamma-ray sources by detecting narrow angle anisotropies in the high energy muon background radiation are considered.
Edwards Philip G.
Protheroe Raymond J.
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