Citations per year, relative to E. G. Berezhko E. G. Berezhko (= 1×)
peers
R. van Lieshout
Countries citing papers authored by E. G. Berezhko
Since
Specialization
Citations
This map shows the geographic impact of E. G. Berezhko's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by E. G. Berezhko with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. G. Berezhko more than expected).
This network shows the impact of papers produced by E. G. Berezhko. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by E. G. Berezhko. The network helps show where E. G. Berezhko may publish in the future.
Co-authorship network of co-authors of E. G. Berezhko
This figure shows the co-authorship network connecting the top 25 collaborators of E. G. Berezhko.
A scholar is included among the top collaborators of E. G. Berezhko based on the total number of
citations received by their joint publications. Widths of edges
represent the number of papers authors have co-authored together.
Node borders
signify the number of papers an author published with E. G. Berezhko. E. G. Berezhko is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Berezhko, E. G., et al.. (1998). Regular acceleration of particles at the fronts of interplanetary shock waves. Astronomy Letters. 24(1). 122–130.6 indexed citations
7.
Berezhko, E. G., et al.. (1996). A self-consistent model for the acceleration of solar-wind protons and generation of Alfvën turbulence by an interplanetary shock wave. Astronomy Letters. 22. 260.2 indexed citations
8.
Berezhko, E. G., et al.. (1996). Cosmic ray acceleration in supernova remnants. 82(1). 1–21.15 indexed citations
9.
Berezhko, E. G., et al.. (1995). The Self-Consistent Model for Acceleration of Solar Wind Protons by the Interplanetary Shock Waves and Coupled Alfvén Waves Generation. ICRC. 4. 357–360.1 indexed citations
10.
Drury, L. O’C., H. J. Voêlk, & E. G. Berezhko. (1995). Existence and interpretation of smooth cosmic-ray dominated shock structures in supernova remnants.. A&A. 299. 222.1 indexed citations
11.
Berezhko, E. G.. (1994). Generation of ultrahigh-energy cosmic rays in the surroundings of pulsars. Astronomy Letters. 20(1). 75–79.7 indexed citations
12.
Berezhko, E. G., et al.. (1993). Spectrum of cosmic ray intensity fluctuations in the solar activity cycle. Astronomy Letters. 19(8). 304–305.2 indexed citations
13.
Berezhko, E. G., et al.. (1991). Shock wave modification for different regimes of cosmic ray acceleration. 55(10). 2063–2065.2 indexed citations
14.
Berezhko, E. G.. (1990). Generation of Magnetohydrodynamic Waves in Interplanetary Plasma by Streams of Solar Cosmic-Rays. 16. 483.2 indexed citations
15.
Berezhko, E. G. & С. А. Стародубцев. (1988). Nature of the dynamics of the cosmic-ray fluctuation spectrum. 52. 2361–2363.2 indexed citations
16.
Berezhko, E. G.. (1986). Instability in a shock propagating through gas with a cosmic-ray component. 12. 352–354.3 indexed citations
17.
Berezhko, E. G.. (1981). Acceleration of charged particles in a cosmic-phase shear flow. 33. 399–401.
18.
Berezhko, E. G., et al.. (1981). Kinetic Consideration of Charged Particle Acceleration Process in Shearing Flows of Collisionless Plasma. 7. 636.1 indexed citations
19.
Berezhko, E. G.. (1981). On Acceleration Possibility of Charged Particles Under Cosmic Plasma Shearing Flows. ICRC. 3. 506.1 indexed citations
20.
Berezhko, E. G. & Г. Ф. Крымский. (1981). Kinetic analysis of the charged-particle acceleration process in collisionless plasma shear flows. 7. 352.
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive
bibliographic database. While OpenAlex provides broad and valuable coverage of the global
research landscape, it—like all bibliographic datasets—has inherent limitations. These include
incomplete records, variations in author disambiguation, differences in journal indexing, and
delays in data updates. As a result, some metrics and network relationships displayed in
Rankless may not fully capture the entirety of a scholar's output or impact.