Wolf‐Christian Müller
- Astronomy and Astrophysics top 2%
- Computational Mechanics top 2%
- Molecular Biology
- Nuclear and High Energy Physics top 10%
- Global and Planetary Change
- Co-authors
- D. BiskampRoland GrappinDaniele CaratiAngela BusseJ. PrattO. AgulloBernard KnaepenRainer Grauer
- Topics
- Solar and Space Plasma Dynamics (32 papers)Ionosphere and magnetosphere dynamics (16 papers)Fluid Dynamics and Turbulent Flows (15 papers)
- Partner nations
- GermanyFranceUnited Kingdom
In The Last Decade
Wolf‐Christian Müller
37 papers receiving 1.2k citations
Peers
Comparison fields: 5 of 39
- Astronomy and Astrophysics 1.0k
- Computational Mechanics 422
- Molecular Biology 421
- Nuclear and High Energy Physics 126
- Global and Planetary Change 78
Countries citing papers authored by Wolf‐Christian Müller
This map shows the geographic impact of Wolf‐Christian Müller'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 Wolf‐Christian Müller with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Wolf‐Christian Müller more than expected).
Fields of papers citing papers by Wolf‐Christian Müller
This network shows the impact of papers produced by Wolf‐Christian Müller. 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 Wolf‐Christian Müller. The network helps show where Wolf‐Christian Müller may publish in the future.
Co-authorship network of co-authors of Wolf‐Christian Müller
This figure shows the co-authorship network connecting the top 25 collaborators of Wolf‐Christian Müller. A scholar is included among the top collaborators of Wolf‐Christian Müller 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 Wolf‐Christian Müller. Wolf‐Christian Müller 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 | 1 | |
| 3 | 2 | |
| 4 | 8 | |
| 5 | 2 | |
| 6 | 2 | |
| 7 | 14 | |
| 8 | 18 | |
| 9 | 28 | |
| 10 | 22 | |
| 11 | 21 | |
| 12 | 6 | |
| 13 | 1 | |
| 14 | 2 | |
| 15 | 6 | |
| 16 | 1 | |
| 17 | 159 | |
| 18 | The residual energy in freely decaying magnetohydrodynamic turbulence. Invited paper | 1 |
| 19 | 121 | |
| 20 | 55 |
About Wolf‐Christian Müller
Wolf‐Christian Müller is a scholar working on Astronomy and Astrophysics, Computational Mechanics and Global and Planetary Change, having authored 39 papers that have together received 1.2k indexed citations. Recurring topics across this work include Solar and Space Plasma Dynamics (32 papers), Ionosphere and magnetosphere dynamics (16 papers) and Fluid Dynamics and Turbulent Flows (15 papers). The work is most often cited by research in Astronomy and Astrophysics (1.0k citations), Computational Mechanics (422 citations) and Nuclear and High Energy Physics (126 citations). Wolf‐Christian Müller has collaborated with scholars based in Germany, France and United Kingdom. Frequent co-authors include D. Biskamp, Roland Grappin, Daniele Carati, Angela Busse, J. Pratt, O. Agullo, Bernard Knaepen, Rainer Grauer, Holger Homann and Andrea Verdini. Their work appears in journals such as Physical Review Letters, The Astrophysical Journal and Journal of Fluid Mechanics.
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.