This map shows the geographic impact of A. Soutoul'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 A. Soutoul with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Soutoul more than expected).
This network shows the impact of papers produced by A. Soutoul. 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 A. Soutoul. The network helps show where A. Soutoul may publish in the future.
Co-authorship network of co-authors of A. Soutoul
This figure shows the co-authorship network connecting the top 25 collaborators of A. Soutoul.
A scholar is included among the top collaborators of A. Soutoul 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 A. Soutoul. A. Soutoul is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Птускин, В. С. & A. Soutoul. (1998). Decaying cosmic ray nuclei in the local interstellar medium. 337(3). 859–865.19 indexed citations
3.
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
4.
Птускин, В. С. & A. Soutoul. (1995). Decaying Cosmic Ray Nuclei as a Probe of the Local Interstellar Medium. ICRC. 3. 132.1 indexed citations
5.
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
6.
Птускин, В. С. & A. Soutoul. (1990). Cosmic rays in the cloudy interstellar medium: production of secondary nuclei. 237(2). 445–453.8 indexed citations
7.
Webber, W. R. & A. Soutoul. (1989). The (C-13)/(C-12) ratio in cosmic ray sources. NASA Technical Reports Server (NASA). 215(1). 128–130.2 indexed citations
Ferrando, P., P. Goret, L. Koch-Miramond, N. Pétrou, & A. Soutoul. (1985). A new analysis of cosmic ray isotopes at 3 GeV/n from HEA03-C2 data. NASA Technical Reports Server (NASA). 2. 96.1 indexed citations
11.
Soutoul, A., J. Engelmann, P. Ferrando, et al.. (1985). Charge and energy dependence of the residence time of cosmic ray nuclei below 15 GeV/nucleon. NASA Technical Reports Server (NASA). 2. 8.2 indexed citations
12.
Lund, N., B. Peters, I. L. Rasmussen, et al.. (1983). The Isotopic Composition of the Cosmic Rays at Energies above 2 Gev/n. International Cosmic Ray Conference. 9. 135.1 indexed citations
13.
Koch-Miramond, L., J. Engelmann, P. Goret, et al.. (1983). Energy spectra of cosmic rays at source as derived from the French-Danish experiment on HEAO-3.. International Cosmic Ray Conference. 2. 219.1 indexed citations
Soutoul, A., J. Engelmann, P. Goret, et al.. (1981). Isotope Analysis Using the Geomagnetic Method. International Cosmic Ray Conference. 9. 105–108.2 indexed citations
16.
Engelmann, J., P. Goret, E. Juliusson, et al.. (1981). The elemental composition of cosmic rays from Be to Zn as measured by the French Danish instrument on HEAO-3. ICRC. 2. 17.8 indexed citations
17.
Perron, C., J. Engelmann, P. Goret, et al.. (1981). Interpretation of the elemental abundances measured by the French-Danish experiment on HEAO-3 - Interstellar propagation and derivation of source abundances. ICRC. 9. 118–121.2 indexed citations
Pétrou, N. & A. Soutoul. (1977). On the Residual Atmosphere Traversed by Cosmic Rays at Large Zenith Angles at Satellite Altitude. ICRC. 11. 273.1 indexed citations
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.