A. D. Erlykin
About
In The Last Decade
A. D. Erlykin
31 papers receiving 264 citations
Peers
Comparison fields: 5 of 29
- Nuclear and High Energy Physics 223
- Astronomy and Astrophysics 149
- Atmospheric Science 29
- Global and Planetary Change 21
- Pulmonary and Respiratory Medicine 11
Countries citing papers authored by A. D. Erlykin
This map shows the geographic impact of A. D. Erlykin'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. D. Erlykin with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. D. Erlykin more than expected).
Fields of papers citing papers by A. D. Erlykin
This network shows the impact of papers produced by A. D. Erlykin. 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. D. Erlykin. The network helps show where A. D. Erlykin may publish in the future.
Co-authorship network of co-authors of A. D. Erlykin
This figure shows the co-authorship network connecting the top 25 collaborators of A. D. Erlykin. A scholar is included among the top collaborators of A. D. Erlykin 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. D. Erlykin. A. D. Erlykin is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 5 | |
| 3 | 8 | |
| 4 | 15 | |
| 5 | 1 | |
| 6 | 24 | |
| 7 | 20 | |
| 8 | 26 | |
| 9 | 1 | |
| 10 | 1 | |
| 11 | 21 | |
| 12 | 1 | |
| 13 | The origin of PeV cosmic rays | 2 |
| 14 | 'FINE STRUCTURE' IN THE ENERGY SPECTRUM, AND CHANGES IN THE MASS COMPOSITION, OF COSMIC RAYS IN THE ENERGY RANGE 0.3-10 PEV | 1 |
| 15 | 8 | |
| 16 | The gradient of cosmic ray protons in the outer Galaxy. | 1 |
| 17 | 1 | |
| 18 | Hadron Flux Absolute Intensity in the Energy Range 2. 10**11 - 2. 10**12 EV at the Mountain Level | 1 |
| 19 | 11 | |
| 20 | Investigation of cascades, produced by high energy muons | 1 |
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.