W. R. Webber
About
In The Last Decade
W. R. Webber
270 papers receiving 6.2k citations
Hit Papers
Peers
Comparison fields: 5 of 127
- Astronomy and Astrophysics 5.3k
- Nuclear and High Energy Physics 2.4k
- Atmospheric Science 710
- Cognitive Neuroscience 705
- Pulmonary and Respiratory Medicine 630
Countries citing papers authored by W. R. Webber
This map shows the geographic impact of W. R. Webber'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 W. R. Webber with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W. R. Webber more than expected).
Fields of papers citing papers by W. R. Webber
This network shows the impact of papers produced by W. R. Webber. 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 W. R. Webber. The network helps show where W. R. Webber may publish in the future.
Co-authorship network of co-authors of W. R. Webber
This figure shows the co-authorship network connecting the top 25 collaborators of W. R. Webber. A scholar is included among the top collaborators of W. R. Webber 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 W. R. Webber. W. R. Webber is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | Analyses of Voyager 2 Plasma Observations in the Heliosheath: Near the Heliospheric Current Sheet and Streamer Belt | 1 |
| 2 | Diffusion and nuclear fragmentation of cosmic rays: choice of galactic model | 0 |
| 3 | Studies of Anomalous Cosmic Ray Hydrogen in the Outer Heliosphere | 3 |
| 4 | Interplanetary E>70 MeV Cosmic Ray Radial and Latitudinal Gradients | 1 |
| 5 | The Nitrogen Abundance in the Cosmic Ray Source | 1 |
| 6 | Energetic storm particle events in the outer heliosphere | 5 |
| 7 | High energy cosmic ray charge and energy spectra measurements | 3 |
| 8 | Measurements of cosmic ray H-2 and He-3 nuclei above 100 MeV/nuc using a balloon borne telescope | 3 |
| 9 | Solar Proton Propagation Characteristics Out to 16 AU | 1 |
| 10 | Comparative energy spectra of z equals 3-8 nuclei in the energy range 200 MeV/nuc to 3 GeV/nuc | 2 |
| 11 | Galactic Cosmic Ray Observations in the Distant Heliosphere | 3 |
| 12 | a Measurement of the Radial Gradient of the Low Energy Anomalous Oxygen Component from 1-16 AU | 4 |
| 13 | A Measurement of the Interplanetary Radial Gradient of Low-energy Oxygen Nuclei from 1-10 Au and Implications of this Measurement | 5 |
| 14 | Observations of galactic cosmic ray energy spectra between 1 and 9 A.U. | 1 |
| 15 | Solar cosmic ray events at large radial distances from the sun | 3 |
| 16 | Differences in the Spectra of Cosmic Ray Nuclear Species Below~5 GeV/nuc | 1 |
| 17 | Isotopic Composition of Cosmic Ray Nuclei with Z>10 | 1 |
| 18 | Calculation of a realistic gradient as a function of radial distance from the sun | 1 |
| 19 | The Modulation of Galactic Cosmic Rays by Interplanetary Magnetic Fields | 7 |
| 20 | Some implications of the relative spectra of the different charge components in the primary radiation. | 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.