R. P. Lin
About
In The Last Decade
R. P. Lin
501 papers receiving 19.8k citations
Hit Papers
Peers
Comparison fields: 5 of 96
- Astronomy and Astrophysics 20.4k
- Molecular Biology 4.4k
- Nuclear and High Energy Physics 1.9k
- Geophysics 1.9k
- Atmospheric Science 1.1k
Countries citing papers authored by R. P. Lin
This map shows the geographic impact of R. P. Lin'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. P. Lin with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. P. Lin more than expected).
Fields of papers citing papers by R. P. Lin
This network shows the impact of papers produced by R. P. Lin. 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. P. Lin. The network helps show where R. P. Lin may publish in the future.
Co-authorship network of co-authors of R. P. Lin
This figure shows the co-authorship network connecting the top 25 collaborators of R. P. Lin. A scholar is included among the top collaborators of R. P. Lin 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. P. Lin. R. P. Lin is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | A Space Weather Mission to the Earth's 5th Lagrangian Point (L5) | 1 |
| 2 | CINEMA (Cubesat for Ion, Neutral, Electron, MAgnetic fields) | 5 |
| 3 | RHESSI X-ray and Gamma-ray observations of the January 20, 2005 event | 3 |
| 4 | Comparison between impulsive 3He-rich events and energetic electron events | 1 |
| 5 | RHESSI Spectroscopy of Nuclear De-excitation Lines in X-class Flares | 2 |
| 6 | Why was there no Solar Energetic Particle Event Associated with the Gamma-ray-line Flare of 2002 July 23? | 1 |
| 7 | Evidence for Electron Acceleration up to ~300 keV in the Magnetic Reconnection Diffusion Region of the Earth's Magnetotail | 6 |
| 8 | Wind Observations of Foreshock Cavities | 2 |
| 9 | CLUSTER ANALYSIS OF LUNAR MAGNETISM, GRAVITY ANOMALIES, AND TOPOLOGY.S. Frey, | 1 |
| 10 | RHESSE observations of particle acceleration in solar flares | 2 |
| 11 | ELECTRON PROPERTIES AND COULOMB COLLISIONS IN THE SOLAR WIND AT 1 AU: WIND OBSERVATIONS | 2 |
| 12 | The High Energy Solar Spectroscopic Imager (HESSI) Small Explorer mission for the next (2000) solar maximum | 2 |
| 13 | Solar Impulsive Electron Events with Unusual Velocity Dispersions | 1 |
| 14 | Regional Mapping of the Lunar Crustal Magnetic Field: Correlation of Strong Anomalies with Curvilinear Albedo Markings | 2 |
| 15 | Initial Maps of the Crustal Magnetic Field of the Moon Using Lunar Prospector Magnetometer Data | 1 |
| 16 | The upstream region, foreshock and bow shock wave at Halley's Comet from plasma electron measurements | 2 |
| 17 | Lunar Magnetization Concentrations (magcons) Antipodal to Young Large Impact Basins | 1 |
| 18 | Description of the main boundaries seen by the Giotto electron experiment inside the Comet Halley-solar wind interaction regions | 1 |
| 19 | Mapping of lunar surface remanent magnetic fields by electron scattering | 6 |
| 20 | Energetic Solar Electrons Accompanying Type III Bursts Observed at 1 A. U. | 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.