Analysis of Lateral Distribution of Atmospheric Cherenkov Light at High Mountain Altitude Towards Event Reconstruction

<table>Lateral distribution of Cherenkov light flux in EAS produced by primary proton showers in the energy range 1013–1017 eV at Chacaltaya observation level.</table>

International Scholarly Research Notices

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Figure 2

Figure 2: Analysis of Lateral Distribution of Atmospheric Cherenkov Light at High Mountain Altitude Towards Event Reconstruction 