T. W. Scattergood
About
In The Last Decade
T. W. Scattergood
27 papers receiving 406 citations
Peers
Comparison fields: 5 of 39
- Astronomy and Astrophysics 384
- Atmospheric Science 113
- Spectroscopy 54
- Ecology 42
- Atomic and Molecular Physics, and Optics 35
Countries citing papers authored by T. W. Scattergood
This map shows the geographic impact of T. W. Scattergood'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. W. Scattergood with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. W. Scattergood more than expected).
Fields of papers citing papers by T. W. Scattergood
This network shows the impact of papers produced by T. W. Scattergood. 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. W. Scattergood. The network helps show where T. W. Scattergood may publish in the future.
Co-authorship network of co-authors of T. W. Scattergood
This figure shows the co-authorship network connecting the top 25 collaborators of T. W. Scattergood. A scholar is included among the top collaborators of T. W. Scattergood 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. W. Scattergood. T. W. Scattergood 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 | 1 | |
| 3 | Laboratory investigations of the aerosols in the stratosphere of Titan | 1 |
| 4 | 39 | |
| 5 | Recent spectroscopic findings concerning clay/water interactions at low humidity: Possible applications to models of Martian surface reactivity | 2 |
| 6 | 23 | |
| 7 | 67 | |
| 8 | Titan's Organic Haze over the Last Four Billion Years | 1 |
| 9 | Constraining Mars Soil Mineralogical Composition: Palagonite vs. Iron Enriched Smectite Clays | 4 |
| 10 | 18 | |
| 11 | 36 | |
| 12 | 67 | |
| 13 | Shock Formation of N 2 and Organic Compounds in a Primordial NH 3 -CH 4 Atmosphere on Titan | 1 |
| 14 | 5 | |
| 15 | 6 | |
| 16 | 0 | |
| 17 | 8 | |
| 18 | Organic chemistry on Titan | 4 |
| 19 | 37 | |
| 20 | On the Sources of UV Absorption in Spectra of Titan and the Outer Planets | 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.