M. J. Pueschel
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- Magnetic confinement fusion research 83
- Laser-Plasma Interactions and Diagnostics 35
- Astronomy and Astrophysics top 1%
- Ionosphere and magnetosphere dynamics 71
- Solar and Space Plasma Dynamics 31
- Aerospace Engineering top 5%
- Particle accelerators and beam dynamics 5
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- Fusion materials and technologies 10
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- Superconducting Materials and Applications 5
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- Fluid Dynamics and Turbulent Flows 4
- Journals
- Physical Review Letters (12 papers)Monthly Notices of the Royal Astronomical Society (2 papers)Computer Physics Communications (1 paper)
- Partner nations
- United StatesGermanyNetherlands
In The Last Decade
M. J. Pueschel
85 papers receiving 2.2k citations
Peers
Comparison fields: 5 of 41
- Nuclear and High Energy Physics 2.1k
- Astronomy and Astrophysics 1.7k
- Aerospace Engineering 284
- Materials Chemistry 346
- Biomedical Engineering 197
Countries citing papers authored by M. J. Pueschel
This map shows the geographic impact of M. J. Pueschel'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 M. J. Pueschel with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. J. Pueschel more than expected).
Fields of papers citing papers by M. J. Pueschel
This network shows the impact of papers produced by M. J. Pueschel. 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 M. J. Pueschel. The network helps show where M. J. Pueschel may publish in the future.
Co-authorship network
The 25 scholars most cited alongside M. J. Pueschel, 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 | 2025 | 1 | |
| 2 | 2025 | 2 | |
| 3 | 2024 | 5 | |
| 4 | 2024 | 3 | |
| 5 | 2023 | 3 | |
| 6 | 2023 | 3 | |
| 7 | 2023 | 4 | |
| 8 | 2023 | 7 | |
| 9 | 2023 | 11 | |
| 10 | 2022 | 5 | |
| 11 | 2022 | 20 | |
| 12 | 2022 | 14 | |
| 13 | 2022 | 5 | |
| 14 | 2021 | 13 | |
| 15 | 2021 | 8 | |
| 16 | 2019 | 17 | |
| 17 | 2019 | 21 | |
| 18 | 2018 | 31 | |
| 19 | 2018 | 20 | |
| 20 | 2015 | 33 |
About M. J. Pueschel
M. J. Pueschel is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Aerospace Engineering, having authored 88 papers that have together received 2.2k indexed citations. Recurring topics across this work include Magnetic confinement fusion research (83 papers), Ionosphere and magnetosphere dynamics (71 papers), Laser-Plasma Interactions and Diagnostics (35 papers), Solar and Space Plasma Dynamics (31 papers), Fusion materials and technologies (10 papers), Superconducting Materials and Applications (5 papers), Particle accelerators and beam dynamics (5 papers) and Fluid Dynamics and Turbulent Flows (4 papers). The work is most often cited by research in Nuclear and High Energy Physics (2.1k citations), Astronomy and Astrophysics (1.7k citations) and Aerospace Engineering (284 citations). M. J. Pueschel has collaborated with scholars based in United States, Germany and Netherlands. Frequent co-authors include F. Jenko, P. W. Terry, D. R. Hatch, D. Told, W. M. Nevins, H. Doerk, T. Dannert, Matthias Kammerer, T. Görler and B. J. Faber. Their work appears in journals such as Physical Review Letters, Monthly Notices of the Royal Astronomical Society and Computer Physics Communications.
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.