Richard J. Stancliffe
About
In The Last Decade
Richard J. Stancliffe
95 papers receiving 1.9k citations
Peers
Comparison fields: 5 of 52
- Astronomy and Astrophysics 1.8k
- Instrumentation 579
- Nuclear and High Energy Physics 231
- Geophysics 92
- Computational Mechanics 33
Countries citing papers authored by Richard J. Stancliffe
This map shows the geographic impact of Richard J. Stancliffe'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 Richard J. Stancliffe with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Richard J. Stancliffe more than expected).
Fields of papers citing papers by Richard J. Stancliffe
This network shows the impact of papers produced by Richard J. Stancliffe. 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 Richard J. Stancliffe. The network helps show where Richard J. Stancliffe may publish in the future.
Co-authorship network of co-authors of Richard J. Stancliffe
This figure shows the co-authorship network connecting the top 25 collaborators of Richard J. Stancliffe. A scholar is included among the top collaborators of Richard J. Stancliffe 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 Richard J. Stancliffe. Richard J. Stancliffe 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 | 6 | |
| 3 | 5 | |
| 4 | 6 | |
| 5 | 18 | |
| 6 | 21 | |
| 7 | 18 | |
| 8 | 121 | |
| 9 | VizieR Online Data Catalog: Low-mass helium white dwarfs evolutionary models (Istrate+, 2016) | 1 |
| 10 | 56 | |
| 11 | 43 | |
| 12 | 5 | |
| 13 | 53 | |
| 14 | 18 | |
| 15 | Why Do Low-Mass Stars Become Red Giants? | 9 |
| 16 | STARS: A Stellar Evolution Code | 2 |
| 17 | 41 | |
| 18 | 0 | |
| 19 | 1 | |
| 20 | A convective model consistent with chemistry | 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.