P. Gouttebroze
About
In The Last Decade
P. Gouttebroze
53 papers receiving 596 citations
Peers
Comparison fields: 5 of 37
- Astronomy and Astrophysics 587
- Atmospheric Science 71
- Artificial Intelligence 48
- Molecular Biology 43
- Atomic and Molecular Physics, and Optics 38
Countries citing papers authored by P. Gouttebroze
This map shows the geographic impact of P. Gouttebroze'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 P. Gouttebroze with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites P. Gouttebroze more than expected).
Fields of papers citing papers by P. Gouttebroze
This network shows the impact of papers produced by P. Gouttebroze. 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 P. Gouttebroze. The network helps show where P. Gouttebroze may publish in the future.
Co-authorship network of co-authors of P. Gouttebroze
This figure shows the co-authorship network connecting the top 25 collaborators of P. Gouttebroze. A scholar is included among the top collaborators of P. Gouttebroze 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 P. Gouttebroze. P. Gouttebroze 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 | 4 | |
| 3 | 13 | |
| 4 | 16 | |
| 5 | The Helium Spectrum in Erupting Solar Prominences | 1 |
| 6 | 15 | |
| 7 | 14 | |
| 8 | 36 | |
| 9 | 15 | |
| 10 | 19 | |
| 11 | Line profiles and intensity ratios in prominence models with a prominence to corona interface | 2 |
| 12 | 17 | |
| 13 | 35 | |
| 14 | 12 | |
| 15 | 12 | |
| 16 | The hydrogen spectrum of model prominences. | 39 |
| 17 | Physical properties of the solar chromosphere deduced from optically thick lines. I - Observations, data reduction, and modelling of an average plage | 2 |
| 18 | 20 | |
| 19 | Doppler Shifts measured in 0 VI line from OSO-B observations above and in the vicinity of plage Mc Math 13738. | 1 |
| 20 | Velocity gradients in the solar chromosphere and Mg II line profiles. | 3 |
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.