D. E. Shemansky
About
In The Last Decade
D. E. Shemansky
25 papers receiving 948 citations
Hit Papers
Peers
Comparison fields: 5 of 58
- Astronomy and Astrophysics 877
- Atmospheric Science 250
- Molecular Biology 120
- Atomic and Molecular Physics, and Optics 101
- Spectroscopy 54
Countries citing papers authored by D. E. Shemansky
This map shows the geographic impact of D. E. Shemansky'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 D. E. Shemansky with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. E. Shemansky more than expected).
Fields of papers citing papers by D. E. Shemansky
This network shows the impact of papers produced by D. E. Shemansky. 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 D. E. Shemansky. The network helps show where D. E. Shemansky may publish in the future.
Co-authorship network of co-authors of D. E. Shemansky
This figure shows the co-authorship network connecting the top 25 collaborators of D. E. Shemansky. A scholar is included among the top collaborators of D. E. Shemansky 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 D. E. Shemansky. D. E. Shemansky is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | Deriving the Structure and Composition of Enceladus’ Plume from Cassini UVIS Observations | 1 |
| 2 | 14 | |
| 3 | 158 | |
| 4 | Energy Deposition Processes in Titan's Upper Atmosphere | 1 |
| 5 | Atmospheric Structure of Saturn and Titan: Results from the Cassini UVIS Experiment | 1 |
| 6 | Cassini UltraViolet Imaging Spectrograph (UVIS) Observations of Enceladus' Plume | 1 |
| 7 | 5 | |
| 8 | Cassini UVIS Observatory Phase spectral imaging of the Saturn system | 1 |
| 9 | 37 | |
| 10 | 30 | |
| 11 | 121 | |
| 12 | 44 | |
| 13 | The Evidence Against an Inner Solar System Source of Atomic Hydrogen | 3 |
| 14 | 4 | |
| 15 | Helium in Collisional Equilibrium with an Electron Gas | 1 |
| 16 | Ion Partitioning in the Io Torus: Voyager I PLS vs. UVS Experiments | 1 |
| 17 | 20 | |
| 18 | 37 | |
| 19 | A Deficiency of OIII in the Io Plasma Torus. | 19 |
| 20 | Radial Dependence of the Io Plasma Torus Spectrum in the EUV. | 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.