R. L. McNutt
About
In The Last Decade
R. L. McNutt
224 papers receiving 7.5k citations
Hit Papers
Peers
Comparison fields: 5 of 94
- Astronomy and Astrophysics 7.7k
- Molecular Biology 2.2k
- Atmospheric Science 1.0k
- Geophysics 487
- Aerospace Engineering 373
Countries citing papers authored by R. L. McNutt
This map shows the geographic impact of R. L. McNutt'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. L. McNutt with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. L. McNutt more than expected).
Fields of papers citing papers by R. L. McNutt
This network shows the impact of papers produced by R. L. McNutt. 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. L. McNutt. The network helps show where R. L. McNutt may publish in the future.
Co-authorship network of co-authors of R. L. McNutt
This figure shows the co-authorship network connecting the top 25 collaborators of R. L. McNutt. A scholar is included among the top collaborators of R. L. McNutt 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. L. McNutt. R. L. McNutt 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 | 7 | |
| 3 | 4 | |
| 4 | 17 | |
| 5 | Planetary Science with an Interstellar Probe | 0 |
| 6 | 12 | |
| 7 | The Plasma Instrument for Magnetic Sounding (PIMS) for the Europa Mission | 0 |
| 8 | 28 | |
| 9 | Intense energetic-electron flux enhancements in Mercury's magnetosphere: An integrated view with high-resolution observations from MESSENGER | 1 |
| 10 | Escape of Pluto's Atmosphere: In Situ Measurements from the Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) instrument on New Horizons and Remote Observations from the Chandra X-ray observatory | 0 |
| 11 | What Happened to the High-Energy (> 100 keV) Particles at Mercury? | 1 |
| 12 | MESSENGER Observations of Magnetotail Dynamics at Mercury | 1 |
| 13 | Mercury Color and Albedo: New Insights from MESSENGER | 1 |
| 14 | Enabling Decadal Survey Science Goals for Primitive Bodies Using Radioisotope Electric Propulsion | 1 |
| 15 | PARIS: A new class of missions to explore the Trojan asteroids and outer solar system | 1 |
| 16 | MESSENGER: The Discovery Mission to Mercury | 2 |
| 17 | The MESSENGER Spacecraft and Payload | 3 |
| 18 | Spatial Gradients, Energy Spectra and Anisotropies of Ions ≥ 30 keV at CIR Shocks from 1 to 50 AU | 10 |
| 19 | Energetic Particle Activity in the Heliosphere 1991-1995 | 6 |
| 20 | The X-Ray/Gamma-Ray Spectrometer for the NEAR Mission | 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.