R. E. Vogt
About
In The Last Decade
R. E. Vogt
42 papers receiving 2.1k citations
Hit Papers
Peers
Comparison fields: 5 of 65
- Astronomy and Astrophysics 1.7k
- Atomic and Molecular Physics, and Optics 737
- Nuclear and High Energy Physics 472
- Ocean Engineering 448
- Geophysics 231
Countries citing papers authored by R. E. Vogt
This map shows the geographic impact of R. E. Vogt'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 R. E. Vogt with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. E. Vogt more than expected).
Fields of papers citing papers by R. E. Vogt
This network shows the impact of papers produced by R. E. Vogt. 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 R. E. Vogt. The network helps show where R. E. Vogt may publish in the future.
Co-authorship network of co-authors of R. E. Vogt
This figure shows the co-authorship network connecting the top 25 collaborators of R. E. Vogt. A scholar is included among the top collaborators of R. E. Vogt 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 R. E. Vogt. R. E. Vogt is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 45 | |
| 2 | 21 | |
| 3 | 7 | |
| 4 | 16 | |
| 5 | 37 | |
| 6 | 13 | |
| 7 | 21 | |
| 8 | Neutral Particle Background in Cosmic Ray Telescopes Composed of Silicon Solid State Detectors | 2 |
| 9 | The elemental composition of 4-30 MeV/nuc cosmic ray nuclei with Z between 1 and 8 | 1 |
| 10 | Observations of low energy interplanetary electrons | 4 |
| 11 | 30 | |
| 12 | The energy spectrum of 0.16 to 3 MeV electrons during solar quiet times | 1 |
| 13 | Observations of Low Energy Hydrogen and Helium Isotopes During Solar Quiet Times | 2 |
| 14 | Observations of the ratio of low-energy cosmic-ray positrons and electrons during solar quiet times | 1 |
| 15 | Solar modulation of cosmic-ray protons and He nuclei | 6 |
| 16 | Measurements of the Flux of Low-Energy Solar-Flare Positrons | 0 |
| 17 | 11 | |
| 18 | 12 | |
| 19 | FLUX AND ENERGY SPECTRA OF PRIMARY COSMIC RAY PROTONS FROM 70 TO 400 Mev | 2 |
| 20 | SOME PROPERTIES OF THE PRIMARY COSMIC RAY ELECTRONS | 3 |
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.