Bruno Bézard
About
In The Last Decade
Bruno Bézard
241 papers receiving 8.0k citations
Peers
Comparison fields: 5 of 70
- Astronomy and Astrophysics 6.9k
- Atmospheric Science 4.0k
- Spectroscopy 1.5k
- Global and Planetary Change 1.1k
- Atomic and Molecular Physics, and Optics 749
Countries citing papers authored by Bruno Bézard
This map shows the geographic impact of Bruno Bézard'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 Bruno Bézard with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Bruno Bézard more than expected).
Fields of papers citing papers by Bruno Bézard
This network shows the impact of papers produced by Bruno Bézard. 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 Bruno Bézard. The network helps show where Bruno Bézard may publish in the future.
Co-authorship network of co-authors of Bruno Bézard
This figure shows the co-authorship network connecting the top 25 collaborators of Bruno Bézard. A scholar is included among the top collaborators of Bruno Bézard 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 Bruno Bézard. Bruno Bézard is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 0 | |
| 3 | 9 | |
| 4 | 0 | |
| 5 | 2 | |
| 6 | 3 | |
| 7 | 36 | |
| 8 | 0 | |
| 9 | 18 | |
| 10 | 63 | |
| 11 | Variability of SO2 and HDO at the cloudtop of Venus from high-resolution infrared spectroscopy | 2 |
| 12 | Determination of Jupiter's N/H ratio from FTS observations at 5 micron. | 1 |
| 13 | H_2O and CO_2 in the Upper Atmospheres of the Giant Planets | 3 |
| 14 | High Resolution Spectroscopy of the GRS and NEB Hot Spots of Jupiter Following Galileo Observations | 1 |
| 15 | Spectro-Imaging of the Dark Side of Venus in the 1.27 μm O 2 Emission with an Imaging FTS | 1 |
| 16 | Intense Localized Near-Infrared Oxygen Airglow on the Venus Night Side | 1 |
| 17 | High-Resolution Spectroscopy of Venus's Night Side in the 2.3, 1.7, and 1.1-1.3μm Windows | 1 |
| 18 | High-Resolution Spectroscopy of Saturn at 5 micrometers II. Cloud Structure and Gaseous Composition | 3 |
| 19 | The Abundance of C 2 H 2 and C 2 H 6 on Saturn Derived from Voyager IRIS Data | 1 |
| 20 | The C/H Ratio in Jupiter from the Voyager Experiment. | 5 |
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.