M. Velli
About
In The Last Decade
M. Velli
162 papers receiving 4.7k citations
Hit Papers
Peers
Comparison fields: 5 of 46
- Astronomy and Astrophysics 5.0k
- Molecular Biology 1.5k
- Nuclear and High Energy Physics 578
- Artificial Intelligence 299
- Computational Mechanics 208
Countries citing papers authored by M. Velli
This map shows the geographic impact of M. Velli'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. Velli with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Velli more than expected).
Fields of papers citing papers by M. Velli
This network shows the impact of papers produced by M. Velli. 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. Velli. The network helps show where M. Velli may publish in the future.
Co-authorship network of co-authors of M. Velli
This figure shows the co-authorship network connecting the top 25 collaborators of M. Velli. A scholar is included among the top collaborators of M. Velli 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. Velli. M. Velli is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 2 | |
| 2 | 8 | |
| 3 | 2 | |
| 4 | 20 | |
| 5 | 3 | |
| 6 | 66 | |
| 7 | 6 | |
| 8 | 14 | |
| 9 | 22 | |
| 10 | 7 | |
| 11 | 4 | |
| 12 | 19 | |
| 13 | 2 | |
| 14 | 31 | |
| 15 | 89 | |
| 16 | 11 | |
| 17 | 23 | |
| 18 | Large-Eddy Simulations of Magnetohydrodynamic Turbulence in Heliophysics and Astrophysics | 47 |
| 19 | 17 | |
| 20 | Origin of Heliospheric Magnetic Field Polarity Inversion at High Latitudes | 1 |
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.