R. H. Brown
About
In The Last Decade
R. H. Brown
273 papers receiving 7.7k citations
Peers
Comparison fields: 5 of 123
- Astronomy and Astrophysics 7.2k
- Atmospheric Science 2.5k
- Ecology 1.2k
- Geophysics 590
- Molecular Biology 424
Countries citing papers authored by R. H. Brown
This map shows the geographic impact of R. H. Brown'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. H. Brown with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. H. Brown more than expected).
Fields of papers citing papers by R. H. Brown
This network shows the impact of papers produced by R. H. Brown. 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. H. Brown. The network helps show where R. H. Brown may publish in the future.
Co-authorship network of co-authors of R. H. Brown
This figure shows the co-authorship network connecting the top 25 collaborators of R. H. Brown. A scholar is included among the top collaborators of R. H. Brown 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. H. Brown. R. H. Brown 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 | 23 | |
| 3 | 17 | |
| 4 | 5 | |
| 5 | Composition of Phoebe and Iapetus: Bound Water and Possible Deuterated Water | 2 |
| 6 | The Ongoing Evolution of a Long-Lived Anticyclone in Saturn’s Great Storm Region as seen by Cassini/VIMS | 1 |
| 7 | The Surface Composition of Titan | 1 |
| 8 | The Evolution of Saturn's Northern Storm of 2010-2011 and Environs as Viewed by Cassini/VIMS | 2 |
| 9 | VIS-IR spectrograms of Saturn's rings retrieved from Cassini-VIMS radial mosaics | 2 |
| 10 | Spectral properties of fluvial terrain on Titan: An update | 1 |
| 11 | Morphology of valley systems on Titan - a comparative study | 1 |
| 12 | Through a Glass Darkly: Saturn's Enigmatic B Ring | 1 |
| 13 | Deconvolution of Cassini VIMS Titan Cubes into Atmospheric Spectral Scattering, Surface Topographic, and Surface Spectroscopic Components | 1 |
| 14 | Near-Infrared Spectroscopy of Trojan Asteroids | 1 |
| 15 | Near-Infrared Spectroscopy of Trojan Asteroids: Implications for the Evolution of the Solar System | 3 |
| 16 | Soil and water engineering | 1 |
| 17 | Volatiles on Icy Satellites: Europa's Trailing Side | 2 |
| 18 | The Dark Side of Iapetus. | 1 |
| 19 | Near-Infrared Spectrophotometry of the Uranian Satellites. | 1 |
| 20 | The rotation period of Neptune. | 8 |
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.