W. Gentner
About
In The Last Decade
W. Gentner
62 papers receiving 885 citations
Peers
Comparison fields: 5 of 70
- Astronomy and Astrophysics 453
- Geophysics 413
- Atmospheric Science 339
- Geochemistry and Petrology 138
- Nuclear and High Energy Physics 120
Countries citing papers authored by W. Gentner
This map shows the geographic impact of W. Gentner'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. Gentner with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W. Gentner more than expected).
Fields of papers citing papers by W. Gentner
This network shows the impact of papers produced by W. Gentner. 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. Gentner. The network helps show where W. Gentner may publish in the future.
Co-authorship network of co-authors of W. Gentner
This figure shows the co-authorship network connecting the top 25 collaborators of W. Gentner. A scholar is included among the top collaborators of W. Gentner 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. Gentner. W. Gentner is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 3 | |
| 2 | 0 | |
| 3 | 1 | |
| 4 | 13 | |
| 5 | The long-term average of the galactic cosmic-ray iron group composition studied by the track method. | 3 |
| 6 | Density and Chemistry of Interplanetary Dust Particles, Derived From Measurements of Lunar Microcraters | 7 |
| 7 | Microcraters of lunar samples. | 5 |
| 8 | Techniques for Identification of VH Ions From Their Etchable Tracks in Minerals. | 1 |
| 9 | Enrichment of volatile elements in Muong Nong-type tektites: clues for their formation history? | 13 |
| 10 | Microcraters on Apollo 15 and 16 samples and corresponding cosmic dust fluxes | 20 |
| 11 | Rare Gases and Ion Tracks in Individual Components and Bulk Samples of Apollo 14 and 15 Fines and Fragmental Rocks | 2 |
| 12 | Some limits on the micrometeoroid flux at 1 au imposed by lunar erosion rates. | 2 |
| 13 | Micromoldavites from the Bavarian Molasse. | 3 |
| 14 | 2 | |
| 15 | 10 | |
| 16 | 31 | |
| 17 | 9 | |
| 18 | 5 | |
| 19 | 1 | |
| 20 | [Considerations on protective screen from a 25 GeV proton-synchroton]. | 2 |
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.