ijmpa˙paper International Journal of Modern Physics A c ○ World Scientific Publishing Company
The energy spectrum of primary cosmic rays with ultra–high energies based on the Yakutsk EAS Array data is presented. For the largest events values of S600 and axis coordinates have been obtained using revised lateral distribution function. The affect of the arrival time distribution at several axis...
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Format: | Text |
Language: | English |
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2004
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Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.254.4061 http://arxiv.org/pdf/astro-ph/0411685v1.pdf |
Summary: | The energy spectrum of primary cosmic rays with ultra–high energies based on the Yakutsk EAS Array data is presented. For the largest events values of S600 and axis coordinates have been obtained using revised lateral distribution function. The affect of the arrival time distribution at several axis distance on estimated density for Yakutsk and AGASA is considered. 1. |
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