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Information Journal Paper

Title

Using the time structure of extensive air showers for cosmic ray mass discrimination

Pages

  33-41

Abstract

 In this research, using CORSIKA simulation code with QGSJETII04 and GHEISHA2002d as high and low energy interaction models respectively, proton and iron Cosmic Ray primaries with 10 17 eV energy and 20-60 o zenith angle are simulated at Tehran observation level (1200m above sea level). By using azimuth angle, arrival time and local coordinates of the muon and electron secondaries as well as rise times of received pulses are calculated. By investigating the rise time as a function of the distance to the Shower Core for different azimuth angle, it is shown that there is an azimuthal asymmetry in the rise time distribution which can be used for mass discrimination of primary Cosmic Rays.

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    APA: Copy

    Rastegarzadeh, Gohar, & Abbasnejad, Hossein. (2020). Using the time structure of extensive air showers for cosmic ray mass discrimination. JOURNAL OF RESEARCH ON MANY BODY SYSTEMS, 9(4 (23) ), 33-41. SID. https://sid.ir/paper/377918/en

    Vancouver: Copy

    Rastegarzadeh Gohar, Abbasnejad Hossein. Using the time structure of extensive air showers for cosmic ray mass discrimination. JOURNAL OF RESEARCH ON MANY BODY SYSTEMS[Internet]. 2020;9(4 (23) ):33-41. Available from: https://sid.ir/paper/377918/en

    IEEE: Copy

    Gohar Rastegarzadeh, and Hossein Abbasnejad, “Using the time structure of extensive air showers for cosmic ray mass discrimination,” JOURNAL OF RESEARCH ON MANY BODY SYSTEMS, vol. 9, no. 4 (23) , pp. 33–41, 2020, [Online]. Available: https://sid.ir/paper/377918/en

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