T. P. Armstrong
About
In The Last Decade
T. P. Armstrong
209 papers receiving 5.5k citations
Peers
Comparison fields: 5 of 104
- Astronomy and Astrophysics 6.0k
- Molecular Biology 1.5k
- Nuclear and High Energy Physics 699
- Atomic and Molecular Physics, and Optics 608
- Geophysics 588
Countries citing papers authored by T. P. Armstrong
This map shows the geographic impact of T. P. Armstrong'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 T. P. Armstrong with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. P. Armstrong more than expected).
Fields of papers citing papers by T. P. Armstrong
This network shows the impact of papers produced by T. P. Armstrong. 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 T. P. Armstrong. The network helps show where T. P. Armstrong may publish in the future.
Co-authorship network of co-authors of T. P. Armstrong
This figure shows the co-authorship network connecting the top 25 collaborators of T. P. Armstrong. A scholar is included among the top collaborators of T. P. Armstrong 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 T. P. Armstrong. T. P. Armstrong is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 25 | |
| 2 | 22 | |
| 3 | Charged Particle Weathering of Saturn's Satellites | 1 |
| 4 | Electron microsignatures from the Saturnian satellites: Cassini MIMI/LEMMS observations | 1 |
| 5 | Energetic particle injections in Saturns magnetosphere | 1 |
| 6 | Energetic Nitrogen Ions within the Inner Magnetosphere of Saturn | 1 |
| 7 | Energetic Electron Beams Measured at Io | 2 |
| 8 | Comparison of the Two Major Solar Proton Events at ULYSSES During March 1991 and May-June 1991 | 1 |
| 9 | Mercury Orbiter: Report of the Science Working Team | 9 |
| 10 | Direct Determination of the Distance to the Hyades Cluster with the Mark III Stellar Interferometer | 3 |
| 11 | Low Energy Ion and Electron Measurements of the March-April 1991 Solar Events by Ulysses | 1 |
| 12 | Electroestatic Charge in Insulating Dust Grains in a Plasma | 1 |
| 13 | Polar Ionospheric Radio Wave Absorption Produced by Solar Flare Energetic Ions | 1 |
| 14 | On the acceleration of thermal coronal ions by flare induced shock waves | 1 |
| 15 | Medium Ion Increases, Solar Flares, and Sector Boundaries | 2 |
| 16 | Recurrent energetic particle events associated with forward/reverse shock pairs near 4 AU in 1978 | 10 |
| 17 | The Quiet-Time Low Energy Nucleon Spectrum during 1975 | 2 |
| 18 | Acceleration of charged particles in oblique MHD shocks | 19 |
| 19 | Observations of quiet-time interplanetary electron enhancements of Jovian origin | 5 |
| 20 | Time variations and angular distributions of alpha particles and medium nuclei for the October 27, 1972 solar-particle event | 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.