Carl Sagan
About
In The Last Decade
Carl Sagan
393 papers receiving 12.9k citations
Hit Papers
Peers
Comparison fields: 5 of 205
- Astronomy and Astrophysics 10.6k
- Atmospheric Science 3.4k
- Aerospace Engineering 1.5k
- Global and Planetary Change 1.3k
- Ecology 1.2k
Countries citing papers authored by Carl Sagan
This map shows the geographic impact of Carl Sagan'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 Carl Sagan with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Carl Sagan more than expected).
Fields of papers citing papers by Carl Sagan
This network shows the impact of papers produced by Carl Sagan. 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 Carl Sagan. The network helps show where Carl Sagan may publish in the future.
Co-authorship network of co-authors of Carl Sagan
This figure shows the co-authorship network connecting the top 25 collaborators of Carl Sagan. A scholar is included among the top collaborators of Carl Sagan 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 Carl Sagan. Carl Sagan is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 0 | |
| 2 | Multispectral imaging of Europa from Galileo's G1 encounter | 1 |
| 3 | Impact-Mediated Chemical Evolution on Titan | 3 |
| 4 | Laboratory Studies of Radiation Chemistry in the Jovian Atmosphere | 3 |
| 5 | Radiation Darkening of CH 4 -clathrate: Implications for the Uranian Satellites | 4 |
| 6 | 1 | |
| 7 | Molecular Analysis of Tholins Produced under Simulated Titan Conditions. | 6 |
| 8 | Reflection Spectra of Simulated Titan Organic Clouds. | 8 |
| 9 | Reflection Spectra of Molten Sulfur: Could Sulfur Liquid be on Io's Surface? | 0 |
| 10 | Signale der Erde : unser Planet stellt sich vor | 2 |
| 11 | Origin of Martian valleys. | 4 |
| 12 | Sulfur Flows on Io. | 20 |
| 13 | Evaporation of Ice-Choked Rivers: Application to Martian Channels. | 2 |
| 14 | McLaughlin and Mars | 7 |
| 15 | Organic Chemistry in the Atmosphere | 19 |
| 16 | Physical Properties of the Particles Composing the Great Martian Dust Storm of 1971 | 4 |
| 17 | High Altitude Aircraft Infrared Spectrometric Observations of Water of Hydration on Mars | 1 |
| 18 | An Elementary Greenhouse Argument for H 2 in the Atmosphere of Titan | 6 |
| 19 | An analysis of the Mariner 4 photography of Mars | 21 |
| 20 | A Windblown Dust Model of Martian Surface Features and Seasonal Changes. | 9 |
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.