Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2093c&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
Scientific paper
Up to now, many projects need to observe high energy electrons above 100 GeV by using the difference of shower development between electron and proton. Monte Carlo simulation is very important in the instrument design and data analysis. The background suppression is strongly dependent on electron and proton shower development. This paper presents the difference of shower simulation between different code and the comparison of simulations with beam test and flight data.
Chang Jaewan
Kasahra K.
Tamura Takeyuki
Torii Shingo
Yoshida Koji
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