M. Bercovitch
About
In The Last Decade
M. Bercovitch
23 papers receiving 253 citations
Peers
Comparison fields: 5 of 30
- Astronomy and Astrophysics 302
- Nuclear and High Energy Physics 89
- Artificial Intelligence 52
- Molecular Biology 44
- Atmospheric Science 40
Countries citing papers authored by M. Bercovitch
This map shows the geographic impact of M. Bercovitch'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 M. Bercovitch with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Bercovitch more than expected).
Fields of papers citing papers by M. Bercovitch
This network shows the impact of papers produced by M. Bercovitch. 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 M. Bercovitch. The network helps show where M. Bercovitch may publish in the future.
Co-authorship network of co-authors of M. Bercovitch
This figure shows the co-authorship network connecting the top 25 collaborators of M. Bercovitch. A scholar is included among the top collaborators of M. Bercovitch 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 M. Bercovitch. M. Bercovitch is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | The Ulysses Cosmic Ray and Solar Particle Investigation | 132 |
| 2 | Muon telescope observations of the solar flare ground level event of 29 September 1989 | 2 |
| 3 | Ground Level Event on August 21, 1979 during STIP Interval VII | 1 |
| 4 | Study of 11 and 22 Year Periodic Variation of Cosmic Ray Diurnal Anisotropy | 4 |
| 5 | Cosmic ray anisotropies at median primary rigidities between 100 and 1000 GV | 8 |
| 6 | Field Gradient and Curvature Drifts and Cosmic Ray Transport into the Solar System | 3 |
| 7 | 29 | |
| 8 | COSMIC RAY DENSITY GRADIENT PERPENDICULAR TO THE ECLIPTIC PLANE. | 1 |
| 9 | Determination of the heliocentric cosmic ray density gradient using neutron monitor data | 14 |
| 10 | 43 | |
| 11 | 11 | |
| 12 | 5 | |
| 13 | 14 | |
| 14 | Atmospheric Effects on Cosmic Ray Monitors | 13 |
| 15 | 4 | |
| 16 | 2 | |
| 17 | Latitude survey in North America. | 10 |
| 18 | Meteorological factors affecting the counting rate of neutron monitors. | 8 |
| 19 | Variability of the energy dependence of the cosmic ray anisotropy | 1 |
| 20 | 16 |
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.