activity
20002022
most citedAll-particle primary energy spectrum in the 3-200 PeV energy range

68 citations · 330 across the 31 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2022★ 15 cited

Formation of the cosmic-ray halo: The role of nonlinear Landau damping

D. O. Chernyshov, V. A. Dogiel, A. V. Ivlev +2

We present a nonlinear model of self-consistent Galactic halo, where the processes of cosmic ray (CR) propagation and excitation/damping of MHD waves are included. The MHD-turbulen…

astro-ph.GA2015★ 8 cited

The radial gradient of cosmic ray intensity in the Galaxy

Anatoly Erlykin, Arnold Wolfendale, Vladimir Dogiel

The dependence of the cosmic ray intensity on Galactocentric distance is known to be much less rapid than that to be thought-to-be sources: supernova remnants. This is an old probl…

astro-ph.GA2014★ 4 cited

The role of the Galactic Halo and the Single Source in the formation of the cosmic ray anisotropy

Anatoly Erlykin, Arnold Wolfendale

The existence of the cosmic ray Halo in our Galaxy has been discussed for more than half a century. If it is real it could help to explain some puzzling features of the cosmic ray…

astro-ph.GA2012★ 22 cited

Cosmic Rays in the Inner Galaxy and the Diffusion Properties of the Interstellar Medium

Anatoly D. Erlykin, Arnold W. Wolfendale

Recent measurements of cosmic gamma ray intensities up to TeV energies have been used to estimate the spectral shape of the parent cosmic ray particles present in the interstellar…

astro-ph.GA2009

Time variability of high energy cosmic rays

A. D. Erlykin, A. W. Wolfendale

Our model involving cosmic ray acceleration in supernova remnants has been used to predict cosmic ray intensities over long periods of time on a statistical basis. If, as is highly…

astro-ph.GA2009

Galactic diffuse gamma-ray flux at the energy about 175 TeV

Romen M. Martirosov, Samvel V. Ter-Antonyan, Anatoly D. Erlykin +4

We present an upper limit of galactic diffuse gamma-ray flux, measured with the GAMMA experiment at energy about 175 TeV. The results were obtained using selection of muon poor ext…