336 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Max Planck Institute for Nuclear PhysicsDE30 papers
- Max Planck SocietyDE20 papers
- Russian Academy of SciencesRU8 papers
- Institute for Nuclear ResearchRU6 papers
- Siberian Branch of the Russian Academy of SciencesRU3 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di TorinoIT2 papers
- Kavli Institute for the Physics and Mathematics of the UniverseJP2 papers
- Lomonosov Moscow State UniversityRU2 papers
- National Institute for AstrophysicsIT2 papers
- New York UniversityUS2 papers
- North Carolina State UniversityUS2 papers
- Norwegian University of Science and TechnologyNO2 papers
9 papers · 2 filters
Spectrum of cosmic rays with energy above eV
S. P. Knurenko, V. P. Egorova, A. V. Glushkov +9
There are some discrepancies in the results on energy spectrum from Yakutsk, AGASA, and HiRes experiments. In this work differential energy spectrum of primary cosmic rays based on…
Fluctuations of Xmax and Primary Particle Mass Composition in the Range of Energy 5 10^{17} - 3 10^{19} ev by Yakutsk Data
S. P. Knurenko, A. A. Ivanov, V. A. Kolosov +3
The experimental distributions of $\Xmax$ obtained with the Yakutsk EAS array at fixed energies of , and eV are analysed. A recen…
Muons with E_th >= 1 Gev and Mass Composition in the Energy Range 10^{18}-10^{20} ev Observed by Yakutsk Eas Array
S. P. Knurenko, V. A. Kolosov, I. T. Makarov +3
The ratio of the muon flux density to charged particle flux density at distances of 300 and 600 m from the shower axis ($\rhom(300)/\rhos(300)$ and $\rhom(600)/\rhos(600)$) is meas…
Influence of Primary Cosmic Radiation Mass Composition on the Estimation of Eas Energy
S. P. Knurenko, A. A. Ivanov, V. A. Kolosov +3
At the Yakutsk EAS array E_em is determined by using measurements of EAS Cherenkov light flux and charged particle flux. It is known from calculations that these characteristics de…
Magnetic Field Amplification in Tycho and other Shell-type Supernova Remnants
H. J. Voelk, E. G. Berezhko, L. T. Ksenofontov
It is shown that amplification of the magnetic field in supernova remnants (SNRs) occurs in all six objects where morphological measurements are presently available in the hard X-r…
The spectrum features of UHECRs below and surrounding GZK
V. P. Egorova, A. V. Glushkov, A. A. Ivanov +10
The energy spectrum of UHECRs is discussed on the basis of the Yakutsk array database analysis. In the region E=0.1 to 30 EeV the showers are detected under trigger-500, while at e…
The theory of synchrotron emission from supernova remnants
E. G. Berezhko, H. J. Völk
The time-dependent nonlinear kinetic theory for cosmic ray (CR) acceleration in supernova remnants (SNRs) is applied studying the properties of the synchrotron emission from SNRs,…
The Contribution of Different Supernova Populations to the Galactic Gamma-Ray Background
E. G. Berezhko, H. J. Voelk
The contribution of Source Cosmic Rays (SCRs), accelerated and still confined in Supernova Remnants (SNRs), to the diffuse high energy \gr emission above 1 GeV from the Galactic di…
Direct evidence of efficient cosmic ray acceleration and magnetic field amplification in Cassiopeia A
E. G. Berezhko, H. J. Voelk
It is shown that the nonlinear kinetic theory of cosmic ray (CR) acceleration in supernova remnants (SNRs) describes the shell-type nonthermal X-ray morphology of Cas A, obtained i…