T. Denk
About
In The Last Decade
T. Denk
56 papers receiving 928 citations
Peers
Comparison fields: 5 of 43
- Astronomy and Astrophysics 934
- Atmospheric Science 318
- Geophysics 129
- Aerospace Engineering 76
- Ecology 61
Countries citing papers authored by T. Denk
This map shows the geographic impact of T. Denk'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. Denk with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. Denk more than expected).
Fields of papers citing papers by T. Denk
This network shows the impact of papers produced by T. Denk. 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. Denk. The network helps show where T. Denk may publish in the future.
Co-authorship network of co-authors of T. Denk
This figure shows the co-authorship network connecting the top 25 collaborators of T. Denk. A scholar is included among the top collaborators of T. Denk 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. Denk. T. Denk is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | Clusters of craters on the Saturnian satellite Dione: morphology and size distribution | 1 |
| 2 | Earth-based and Cassini-spacecraft Observations of Irregular Moons of Jupiter and Saturn | 1 |
| 3 | Iapetus: A Two-step Explanation for its Unique Global Appearance | 1 |
| 4 | Enceladus' South Polar Terrain Geology: New Details from Cassini ISS High Resolution Imaging | 9 |
| 5 | Geology of Saturn's Satellite Rhea on the Basis of the High-Resolution Images from the Targeted Flyby 049 on Aug. 30, 2007 | 4 |
| 6 | Iapetus Imaging During the Targeted Flyby of the Cassini Spacecraft | 5 |
| 7 | Geology and Geomorphology of Rhea: a First Look at the High-Resolution Cassini ISS Images from the Targeted Flyby on Aug. 30, 2007. | 1 |
| 8 | Patterns of Fracture and Tectonic Convergence near the South Pole of Enceladus | 13 |
| 9 | Sizes, Shapes, Relaxation States, And Interior Configurations Of Icy Saturnian Satellites | 2 |
| 10 | The geology of Saturn's satellite Dione observed by Cassini's ISS camera | 2 |
| 11 | Physical and Orbital Properties of Some of Saturn's Small Satellites | 3 |
| 12 | Geological Features and Terrains on Enceladus as seen by Cassini ISS | 2 |
| 13 | The cratering record of the Saturnian satellites Phoebe, Tethys, Dione, and Iapetus in comparison: first results from analysis of the Cassini ISS image data | 16 |
| 14 | Iapetus (1): Size, Topography, Surface Structures, Craters | 9 |
| 15 | A Comparison of the Plasma Bombardment Boundary on Ganymede's Surface to Galileo Imaging Data | 1 |
| 16 | A Recently Active Lineament on Europa | 3 |
| 17 | Europa's color obvserved by Galileo-SSI: yellow mottled terrain on the leading side, brown motled terrain on the trailing side | 2 |
| 18 | Ganymede northern high-latitude frosts: preliminary observations from Galileo SSI data | 2 |
| 19 | The Distribution and Origin of Dark Material in Galileo Regio, Ganymede: New Evidence from Geological Relationships Seen in the Galileo Data | 2 |
| 20 | Multispectral imaging of Europa from Galileo's G1 encounter | 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.