Showing 1–20 of 32 results
/ Date/ Name
Feb 21, 2012On the Anisotropy of E0 >= 5.5$\times$1019 eV Cosmic Rays according to Data of the Pierre Auger CollaborationFeb 23, 2012Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave BackgroundApr 19, 2023Muons in EASs with $E_0 = 10^{19}$ eV according to data of the Yakutsk ArrayApr 25, 2023Muon puzzle in ultra-high energy EASs according to Yakutsk array and Auger experiment dataJan 28, 2023Content of muons in extensive air showers measured by Yakutsk arrayAug 27, 2014Revision of the energy calibration of the Yakutsk EAS arrayJan 19, 2006Upper limit on the ultra-high-energy photon flux from AGASA and Yakutsk dataJun 29, 2023A Direct Comparison of Muon Measurements at the Yakutsk Array and the Pierre Auger ObservatoryJan 21, 2026The puzzle of composition of cosmic rays with energies (2-12.5) EeV according to muon detectors data of the Yakutsk EAS arrayDec 8, 2009The possible feature of the energy spectrum of the primary cosmic rays at ultra-high energiesApr 17, 2023Zenith-Angular Characteristics of Particles in EASs with $E_0 \simeq 10^{18}$ eV According to the Yakutsk Array DataJul 15, 2021Status of the Yakutsk air shower array and future plansNov 7, 2013Variations of the cosmic ray composition at energy above 0.1 EeV as observed by muon detectors of Yakutsk arrayNov 17, 2004Spectrum of cosmic rays with energy above $10^{17}$ eVFeb 27, 2012Dependence of the Energy Spectrum of UHE Cosmic Rays on the Latitude of an Extensive Air Shower ArrayJan 23, 2023Energy Spectrum of Ultrahigh-Energy Cosmic Rays according to Data from Ground-Based Scintillation Detectors of the Yakutsk EAS ArrayApr 25, 2024On the calibration of ultra-high energy EASs at the Yakutsk array and Telescope ArrayJul 23, 2004Cosmic Rays and Solar Insolation as the Main Control Parameters of the Catastrophe Theory of Climatic Response to Orbital VariationsAug 26, 2004The spectrum features of UHECRs below and surrounding GZKOct 1, 2024Explanation to the article "On the calibration of ultra-high energy EASs at the Yakutsk array and Telescope Array"