Volume 10, Issue 1 (Iranian Journal of physics Research, Spring 2010)                   IJPR 2010, 10(1): 47-53 | Back to browse issues page

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University of Semnan
Abstract:   (11792 Views)
Different high energy interaction models are the applied in CORSIKA code to simulate Extensive Air Showers (EAS) generated by Cosmic Rays (CR). In this work the effects of QGSJET01, QGSJETII, DPMJET, SIBYLL models on Xmax and multiplicity of secondary electrons and muons at observation level are studied.
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Type of Study: Research | Subject: General