Åke Nordlund
About
In The Last Decade
Åke Nordlund
227 papers receiving 12.8k citations
Hit Papers
Peers
Comparison fields: 5 of 112
- Astronomy and Astrophysics 12.7k
- Instrumentation 1.7k
- Molecular Biology 1.4k
- Atmospheric Science 978
- Nuclear and High Energy Physics 850
Countries citing papers authored by Åke Nordlund
This map shows the geographic impact of Åke Nordlund'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 Åke Nordlund with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Åke Nordlund more than expected).
Fields of papers citing papers by Åke Nordlund
This network shows the impact of papers produced by Åke Nordlund. 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 Åke Nordlund. The network helps show where Åke Nordlund may publish in the future.
Co-authorship network of co-authors of Åke Nordlund
This figure shows the co-authorship network connecting the top 25 collaborators of Åke Nordlund. A scholar is included among the top collaborators of Åke Nordlund 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 Åke Nordlund. Åke Nordlund is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 8 | |
| 3 | 2 | |
| 4 | 2 | |
| 5 | Supernova driving. II. Compressive ratio in molecular-clou turbulence | 34 |
| 6 | 181 | |
| 7 | Helioseismic Data from Emerging Flux Simulations | 1 |
| 8 | Spontaneous Pore Formation in Magneto-Convection Simulations | 2 |
| 9 | 25 | |
| 10 | Solar Magneto-Convection Simulations | 0 |
| 11 | The Future: Where are We Headed | 1 |
| 12 | Brown dwarfs from turbulent fragmentation | 1 |
| 13 | Magnetoconvection and micropores | 2 |
| 14 | Solar convection and magneto-convection simulations | 1 |
| 15 | Line formation in solar granulation. II. The photospheric Fe abundance | 7 |
| 16 | Seismology of the solar surface regions | 3 |
| 17 | 1 | |
| 18 | What Does the Sun Look Like Beneath the Surface | 1 |
| 19 | 7 | |
| 20 | Grid of model atmospheres for metal-deficient giant stars. II | 14 |
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.