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Title

IDENTIFICATION OF COSMIC RAYS BY THEIR SECONDARY PARTICLE SURFACE DISTRIBUTION

Author(s)

 PURMOHAMMAD DAVOUD

Pages

  -

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Abstract

 DISCRIMINATION OF PRIMARY COSMIC RAYS WHICH PRODUCE EXTENSIVE AIR SHOWERS, LEADS US TO BETTER UNDERSTANDING OF CHEMICAL COMPOSITION OF COSMIC RAYS. IN THE GAMMA RAY ASTRONOMY, THIS WOULD RESULT IN A BETTER SIGNAL TO NOISE RATIO. IN THIS PAPER, A WAVELET ANALYSIS ON THE SURFACE DISTRIBUTION OF SECONDARY ELECTRONS IN MONTE CARLO SIMULATED SHOWERS IS PRESENTED. ALTHOUGH THESE RESULTS REJECT THE MULTIRACIAL BEHAVIOR, AS REPORTED IN SOME WORKS, THE SHAPE OF WAVELET TRANSFORM OF THE DISTRIBUTION PROVIDES A CLUE TO THE PRIMARY TYPE IDENTIFICATION.

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    APA: Copy

    PURMOHAMMAD, DAVOUD. (2005). IDENTIFICATION OF COSMIC RAYS BY THEIR SECONDARY PARTICLE SURFACE DISTRIBUTION. IRAN PHYSICS CONFERENCE. SID. https://sid.ir/paper/906834/en

    Vancouver: Copy

    PURMOHAMMAD DAVOUD. IDENTIFICATION OF COSMIC RAYS BY THEIR SECONDARY PARTICLE SURFACE DISTRIBUTION. 2005. Available from: https://sid.ir/paper/906834/en

    IEEE: Copy

    DAVOUD PURMOHAMMAD, “IDENTIFICATION OF COSMIC RAYS BY THEIR SECONDARY PARTICLE SURFACE DISTRIBUTION,” presented at the IRAN PHYSICS CONFERENCE. 2005, [Online]. Available: https://sid.ir/paper/906834/en

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