Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
This map shows the geographic impact of В. С. Птускин'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 В. С. Птускин with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites В. С. Птускин more than expected).
This network shows the impact of papers produced by В. С. Птускин. 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 В. С. Птускин. The network helps show where В. С. Птускин may publish in the future.
Co-authorship network of co-authors of В. С. Птускин
This figure shows the co-authorship network connecting the top 25 collaborators of В. С. Птускин.
A scholar is included among the top collaborators of В. С. Птускин 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 В. С. Птускин. В. С. Птускин is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Буднев, Н., О. Гресс, L. Pankov, et al.. (2005). Array for detection of EAS by Cherenkov light with area of 1 km2 in Tunka Valley. Bulletin of the Russian Academy of Sciences Physics. 69(3). 395–398.2 indexed citations
7.
Птускин, В. С.. (2005). Origin of galactic cosmic rays: sources, acceleration and propagation (OG-2). CERN Document Server (European Organization for Nuclear Research). 10. 317.2 indexed citations
Sina, R., В. С. Птускин, & E. S. Seo. (2003). The Flux of Cosmic-Ray Deuterons in Simplified Propagation Models. International Cosmic Ray Conference. 4. 1973.1 indexed citations
10.
Птускин, В. С., F. C. Jones, A. Lukasiak, & W. R. Webber. (2001). Diffusion and nuclear fragmentation of cosmic rays: choice of galactic model. International Cosmic Ray Conference. 5. 1947.
11.
Птускин, В. С.. (1999). The modified weighted slab technique: results. ICRC. 4. 291.4 indexed citations
12.
Птускин, В. С., F. C. Jones, J. F. Ormes, & A. Soutoul. (1997). Path-length Distribution for Cosmic Rays in Galactic Diffusion Model. International Cosmic Ray Conference. 4. 261.1 indexed citations
13.
Птускин, В. С., et al.. (1995). Propagation of Cosmic-Rays in a Medium with Magnetic Traps. Astronomy Letters. 21(3). 411–417.6 indexed citations
14.
Птускин, В. С. & A. Soutoul. (1995). Decaying Cosmic Ray Nuclei as a Probe of the Local Interstellar Medium. ICRC. 3. 132.1 indexed citations
15.
Zirakashvili, V. N., et al.. (1991). Cosmic Ray Nonlinear Modulation in the outer Heliosphere. ICRC. 3. 585.1 indexed citations
16.
Птускин, В. С. & A. Soutoul. (1991). Cosmic Rays in the Cloudy Interstellar Medium: Diffusion of Radioactive Nuclei. International Cosmic Ray Conference. 2. 197.1 indexed citations
17.
Птускин, В. С.. (1988). Cosmic-Ray Acceleration by Long-Wave Turbulence. 14. 255.12 indexed citations
18.
Птускин, В. С.. (1986). Hydrodynamics of Interstellar Medium Including Cosmic Rays. 251. 279.1 indexed citations
19.
Птускин, В. С.. (1984). Pressure of a gas of fast charged particles that diffuse in a mediumwith a stochastic magnetic field. Journal of Experimental and Theoretical Physics. 59(2). 281.1 indexed citations
20.
Птускин, В. С., et al.. (1981). The Galactic Center and the Origin of Cosmic Rays. 25. 547.
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.