most citedCosmic Rays with Energy Above 10^{17} ev

4 citations · 4 across the 4 of their papers we have counts for

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astro-ph200760 cited

Muon content of ultra-high-energy air showers: Yakutsk data versus simulations

A. V. Glushkov, I. T. Makarov, M. I. Pravdin +4

We analyse a sample of 33 extensive air showers (EAS) with estimated primary energies above 2\cdot 10^{19} eV and high-quality muon data recorded by the Yakutsk EAS array. We compa…

astro-ph200740 cited

Constraining the fraction of primary gamma rays at ultra-high energies from the muon data of the Yakutsk extensive-air-shower array

A. V. Glushkov, D. S. Gorbunov, I. T. Makarov +4

By making use of the data on the total signal and on the muon component of the air showers detected by the Yakutsk array, we analyze, in the frameworks of the recently suggested ev…

astro-ph2005

Estimate of the Mass Composition of Ultrahigh Energy Cosmic Rays

A. A. Mikhailov, N. N. Efremov, N. S. Gerasimova +3

It is proposed a new approach for estimating the composition of cosmic rays. It is found that the zenith angle distributions and muon components of EAS for energies E>10^19 eV and…

astro-ph20044 cited

Cosmic Rays with Energy Above 10^{17} ev

V. P. Egorova, A. V. Glushkov, A. A. Ivanov +10

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 hav…

astro-ph2004

Characteristics of EAS and Primary Particle Mass Composition in the Energy Region of eV by Yakutsk Data

S. P. Knurenko, V. P. Egorova, A. A. Ivanov +5

In the work the data of the Yakutsk complex EAS array and their comparison with calculation in the case of primary nuclei of different chemical elements are presented. The calculat…

astro-ph2004

Deficit of Ultrahigh Energy Extensive Air Showers

A. A. Mikhailov, N. N. Efremov, I. T. Makarov +2

Arrival directions of extensive air showers by using world data are considered. It is shown that distributions of showers in zenith angle at E>10^{19}eV and E>4.10^{19}eV differ fr…