Average estimations of the shower energy components are presented and their sum gives E sub 0 (Rho sub 600) - an average function of the relation of E sub 0 with the shower size parameter Rho sub 600 measured at the Yakutsk extensive air showers (EAS) array. Using this relation to the EAS spectrum obtained at the Akeno and Yakutsk arrays the energy spectrum of the cosmic ray total flux within 15 lg (E sub 0,eV) 20 by the EAS methods is recovered
A new Cerenkov photon density spectrum measurement is reported. The derivation of the primary cosmic...
A new method of a primary cosmic particle energy measurement with the extensive air shower (EAS) tec...
Submitted to Cornell University’s online archive www.arxiv.org in 1999 by Chihwa Song Post-print sou...
The extensive air showers spectrum on scintillation desity Rko in primary energy region E sub approx...
The Yakutsk Extensive Air Showers (EAS) array was designed for detecting the showers generated by th...
The extensive air showers (EAS) cascade curves from the Cerenkov light lateral distribution measurem...
During the initial period of the Samarkand EAS array operations the showers were selected on the bas...
Fluctuations of the shower maximum depth obtained from analysis of electron and muon fluctuations an...
The Yakutsk array observes the Cherenkov light emitted by UHECR in atmosphere. Recently, an autonomo...
The paper presents results on the longitudinal development of air showers of ultra-high energies obt...
A proposed new method for measuring the Cherenkov light from extensive air showers (EAS) of cosmic r...
Arrival directions of ultra-high energy cosmic rays (UHECRs) in the equatorial system, detected with...
The cosmic ray energy spectrum in the range E-o = 10(15)-10(16) eV (including the region of the stee...
Complex analysis of the Yakutsk array data in order to find air showers produced by photons with ene...
The muon content of extensive air showers (EAS) was measured over the wide primary energy range 10 t...
A new Cerenkov photon density spectrum measurement is reported. The derivation of the primary cosmic...
A new method of a primary cosmic particle energy measurement with the extensive air shower (EAS) tec...
Submitted to Cornell University’s online archive www.arxiv.org in 1999 by Chihwa Song Post-print sou...
The extensive air showers spectrum on scintillation desity Rko in primary energy region E sub approx...
The Yakutsk Extensive Air Showers (EAS) array was designed for detecting the showers generated by th...
The extensive air showers (EAS) cascade curves from the Cerenkov light lateral distribution measurem...
During the initial period of the Samarkand EAS array operations the showers were selected on the bas...
Fluctuations of the shower maximum depth obtained from analysis of electron and muon fluctuations an...
The Yakutsk array observes the Cherenkov light emitted by UHECR in atmosphere. Recently, an autonomo...
The paper presents results on the longitudinal development of air showers of ultra-high energies obt...
A proposed new method for measuring the Cherenkov light from extensive air showers (EAS) of cosmic r...
Arrival directions of ultra-high energy cosmic rays (UHECRs) in the equatorial system, detected with...
The cosmic ray energy spectrum in the range E-o = 10(15)-10(16) eV (including the region of the stee...
Complex analysis of the Yakutsk array data in order to find air showers produced by photons with ene...
The muon content of extensive air showers (EAS) was measured over the wide primary energy range 10 t...
A new Cerenkov photon density spectrum measurement is reported. The derivation of the primary cosmic...
A new method of a primary cosmic particle energy measurement with the extensive air shower (EAS) tec...
Submitted to Cornell University’s online archive www.arxiv.org in 1999 by Chihwa Song Post-print sou...