M. S. Nakwacki
- Astronomy and Astrophysics top 5%
- Molecular Biology
- Nuclear and High Energy Physics
- Artificial Intelligence
- Geophysics
- Co-authors
- S. DassoC. H. MandriniP. DémoulinG. D. R. AttrillL. van Driel‐GesztelyiL. K. HarraD. Falceta-GonçalvesH. A. Elliott
- Topics
- Solar and Space Plasma Dynamics (13 papers)Ionosphere and magnetosphere dynamics (8 papers)Astro and Planetary Science (6 papers)
In The Last Decade
M. S. Nakwacki
14 papers receiving 442 citations
Peers
Comparison fields: 5 of 17
- Astronomy and Astrophysics 452
- Molecular Biology 130
- Nuclear and High Energy Physics 23
- Artificial Intelligence 16
- Geophysics 9
Countries citing papers authored by M. S. Nakwacki
This map shows the geographic impact of M. S. Nakwacki'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. S. Nakwacki with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. S. Nakwacki more than expected).
Fields of papers citing papers by M. S. Nakwacki
This network shows the impact of papers produced by M. S. Nakwacki. 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. S. Nakwacki. The network helps show where M. S. Nakwacki may publish in the future.
Co-authorship network of co-authors of M. S. Nakwacki
This figure shows the co-authorship network connecting the top 25 collaborators of M. S. Nakwacki. A scholar is included among the top collaborators of M. S. Nakwacki 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 M. S. Nakwacki. M. S. Nakwacki is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 5 | |
| 2 | 5 | |
| 3 | Magnetic Field Amplification and Evolution in Turbulent Collisionless Magnetohydrodynamics: An Application to the Intracluster Medium | 46 |
| 4 | 3 | |
| 5 | 1 | |
| 6 | 0 | |
| 7 | 36 | |
| 8 | 2 | |
| 9 | 23 | |
| 10 | 3 | |
| 11 | 63 | |
| 12 | 0 | |
| 13 | 68 | |
| 14 | 110 | |
| 15 | 90 | |
| 16 | Helicity Analysis for Expanding Magnetic Clouds: A Case Study | 3 |
About M. S. Nakwacki
M. S. Nakwacki is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Applied Mathematics, having authored 16 papers that have together received 458 indexed citations. Recurring topics across this work include Solar and Space Plasma Dynamics (13 papers), Ionosphere and magnetosphere dynamics (8 papers) and Astro and Planetary Science (6 papers). The work is most often cited by research in Astronomy and Astrophysics (452 citations), Molecular Biology (130 citations) and Nuclear and High Energy Physics (23 citations). M. S. Nakwacki has collaborated with scholars based in Argentina, Brazil and France. Frequent co-authors include S. Dasso, C. H. Mandrini, P. Démoulin, G. D. R. Attrill, L. van Driel‐Gesztelyi, L. K. Harra, D. Falceta-Gonçalves, H. A. Elliott, G. Kowal and E. M. de Gouveia Dal Pino. Their work appears in journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and Nuclear Physics A.
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.