A. Ruzmaikin
About
In The Last Decade
A. Ruzmaikin
159 papers receiving 3.2k citations
Peers
Comparison fields: 5 of 112
- Astronomy and Astrophysics 2.3k
- Molecular Biology 1.2k
- Atmospheric Science 544
- Global and Planetary Change 511
- Oceanography 376
Countries citing papers authored by A. Ruzmaikin
This map shows the geographic impact of A. Ruzmaikin'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 A. Ruzmaikin with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Ruzmaikin more than expected).
Fields of papers citing papers by A. Ruzmaikin
This network shows the impact of papers produced by A. Ruzmaikin. 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 A. Ruzmaikin. The network helps show where A. Ruzmaikin may publish in the future.
Co-authorship network of co-authors of A. Ruzmaikin
This figure shows the co-authorship network connecting the top 25 collaborators of A. Ruzmaikin. A scholar is included among the top collaborators of A. Ruzmaikin 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 A. Ruzmaikin. A. Ruzmaikin is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 8 | |
| 2 | 32 | |
| 3 | Quasi periodicities in the Fluctuations of the Axisymmetric Solar Magnetic Field from Independent Component Analysis | 1 |
| 4 | 21 | |
| 5 | On the Nature and Persistence of Preferred Longitudes of Solar Activity. | 2 |
| 6 | 12 | |
| 7 | Magnitude of the dynamo-generated magnetic field in solar-type convective zones. | 12 |
| 8 | Differential rotation of the liquid core of the Earth. | 1 |
| 9 | 144 | |
| 10 | Generation of large-scale magnetic fields on Uranus and Neptune by turbulent dynamo mechanism. | 2 |
| 11 | Negative Magnetic Pressure as a Trigger of Largescale Magnetic Instability in the Solar Convective Zone | 4 |
| 12 | The large-scale internal solar magnetic field | 0 |
| 13 | The effect of negative magnetic pressure and the large-scale magnetic field instability in the solar convective zone | 1 |
| 14 | Growth of magnetic-field fluctuations in a turbulent flow | 1 |
| 15 | Magnetic manifestations of solar rotation | 2 |
| 16 | Magnetic field transport in an acoustic turbulence type flow | 3 |
| 17 | Steady-state magnetic field in a periodic flow | 2 |
| 18 | The solar cycle as a strange attractor | 20 |
| 19 | Турбулентное динамо в астрофизике | 6 |
| 20 | The turbulent dynamo in astrophysics | 78 |
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.