T. L. Roush
About
In The Last Decade
T. L. Roush
192 papers receiving 6.8k citations
Hit Papers
Peers
Comparison fields: 5 of 118
- Astronomy and Astrophysics 5.3k
- Atmospheric Science 1.5k
- Artificial Intelligence 1.2k
- Ecology 1.2k
- Aerospace Engineering 579
Countries citing papers authored by T. L. Roush
This map shows the geographic impact of T. L. Roush'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. L. Roush with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. L. Roush more than expected).
Fields of papers citing papers by T. L. Roush
This network shows the impact of papers produced by T. L. Roush. 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. L. Roush. The network helps show where T. L. Roush may publish in the future.
Co-authorship network of co-authors of T. L. Roush
This figure shows the co-authorship network connecting the top 25 collaborators of T. L. Roush. A scholar is included among the top collaborators of T. L. Roush 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. L. Roush. T. L. Roush is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 4 | |
| 2 | 14 | |
| 3 | Spectral Clustering on Mercury Hollows: The Dominici Crater Case | 2 |
| 4 | Dehydration-Rehydration Experiments with Cl Salts Mixed into Mars Analog Materials and the Effects on their VNIR Spectral Properties | 3 |
| 5 | Estimation of visible, near-, and mid-infrared optical constants of dolomite | 3 |
| 6 | Toro Crater: First Evidence for Hesperian Phyllosilicates on Mars | 1 |
| 7 | Estimated Optical Constants of Magnesite (MgCO3) | 1 |
| 8 | Evolution of Water Ice Mound Deposit in "Louth" Crater as Observed by CRISM and HiRISE | 1 |
| 9 | Gypsum Optical Constants in the Visible and Near-infrared: Real and Imagined | 2 |
| 10 | Studies of Planetary Materials Using Cryogenic Reflectance Spectroscopy | 1 |
| 11 | Saturn's rings: Surface composition of particles from new near-infrared observations and reflectance modeling | 1 |
| 12 | Autonomous Science Analyses of Digital Images for Mars Sample Return and Beyond | 7 |
| 13 | Autonomous Science Decisions for Mars Sample Return | 4 |
| 14 | Analysing rock samples for the mars lander | 7 |
| 15 | Near-IR (0.8-2.5 micrometers) Optical Constants of Water Ice at 100K | 1 |
| 16 | Why are Saturn's Inner Satellites so White? | 1 |
| 17 | Characterization of a Mauna Kea Palagonite Using Transmission Electron Microsopy | 3 |
| 18 | Analysis of Martian crustal petrology. | 5 |
| 19 | Multispectral Analysis of the Kasei Vallis - Lunae Planum Region of Mars | 4 |
| 20 | The Effect of Thermal Variations on Reflectance Spectra of Mafic Minerals | 3 |
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.