Correlation of <= 10 TeV Primary Gamma Ray Direction and the Direction of Associated Secondary Muons at Sea Level

Details Correlation of <= 10 TeV Primary Gamma Ray Direction and the Direction of Associated Secondary Muons at Sea Level Correlation of <= 10 TeV Primary Gamma Ray Direction and the Direction of Associated Secondary Muons at Sea Level

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....3.1041p&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

The FLUKA Monte Carlo program is used to predict the angular distributions of the muons which originate from primary cosmic gamma rays and reach sea level. This yields the inherent angular resolution of any instrument utilizing muons to infer properties of gamma ray primaries. Various physical effects are also discussed which affect these distributions in differing proportions.

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