G. Pérès
Impact in
- Astronomy and Astrophysics top 0.5%
- Stellar, planetary, and galactic studies
- Solar and Space Plasma Dynamics
- Astrophysics and Star Formation Studies
- Astro and Planetary Science
- Astrophysical Phenomena and Observations
- Gamma-ray bursts and supernovae
- Ionosphere and magnetosphere dynamics
-
- Astrophysics and Cosmic Phenomena
Papers in
-
- Solar and Space Plasma Dynamics 84
- Stellar, planetary, and galactic studies 72
- Astrophysics and Star Formation Studies 46
- Astrophysical Phenomena and Observations 40
- Astro and Planetary Science 37
- Gamma-ray bursts and supernovae 29
- Ionosphere and magnetosphere dynamics 25
G. Pérès
188 papers receiving 3.4k citations
Peers
Comparison fields: 5 of 89
- Astronomy and Astrophysics 3.0k
- Nuclear and High Energy Physics 476
- Soil Science 243
- Instrumentation 79
- Ecology, Evolution, Behavior and Systematics 176
Countries citing papers authored by G. Pérès
This map shows the geographic impact of G. Pérès'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 G. Pérès with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Pérès more than expected).
Fields of papers citing papers by G. Pérès
This network shows the impact of papers produced by G. Pérès. 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 G. Pérès. The network helps show where G. Pérès may publish in the future.
Co-authorship network
The 25 scholars most cited alongside G. Pérès, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.
All Works
| # | Work | ||
|---|---|---|---|
| 1 | 2022 | 15 | |
| 2 | 2022 | 7 | |
| 3 | 2022 | 18 | |
| 4 | 2022 | 33 | |
| 5 | 2021 | 8 | |
| 6 | 2020 | 52 | |
| 7 | 2018 | 10 | |
| 8 | 2017 | 11 | |
| 9 | 2010 | 18 | |
| 10 | 2010 | 28 | |
| 11 | 2009 | 22 | |
| 12 | 2009 | 16 | |
| 13 | 2007 | 46 | |
| 14 | 2006 | 1 | |
| 15 | 2005 | 19 | |
| 16 | 2005 | 11 | |
| 17 | 2005 | 15 | |
| 18 | 2002 | 9 | |
| 19 | Recent results on the study of the Sun as an X-ray star | 2001 | 1 |
| 20 | The Dynamics Of The Plasma Confined In Coronal Loops Subject To A Random Heating | 1999 | 1 |
About G. Pérès
G. Pérès is a scholar working on Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Geophysics and Soil Science, having authored 192 papers that have together received 3.5k indexed citations. Recurring topics across this work include Solar and Space Plasma Dynamics (84 papers), Stellar, planetary, and galactic studies (72 papers), Astrophysics and Star Formation Studies (46 papers), Astrophysical Phenomena and Observations (40 papers), Astro and Planetary Science (37 papers), Gamma-ray bursts and supernovae (29 papers), Ionosphere and magnetosphere dynamics (25 papers) and Astrophysics and Cosmic Phenomena (20 papers). The work is most often cited by research in Astronomy and Astrophysics (3.0k citations), Nuclear and High Energy Physics (476 citations), Soil Science (243 citations), Instrumentation (79 citations) and Ecology, Evolution, Behavior and Systematics (176 citations). G. Pérès has collaborated with scholars based in Italy, United States and France. Frequent co-authors include F. Reale, S. Orlando, S. Serio, R. Rosner, A. Maggio, G. S. Vaiana, L. Golub, F. Bocchino, G. Micela and C. Argiroffi. Their work appears in journals such as The Astrophysical Journal, Astronomy and Astrophysics, Solar Physics, Monthly Notices of the Royal Astronomical Society and Advances in Space Research.
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.