W. Schaffenberger

545 total citations
13 papers, 307 citations indexed

About

W. Schaffenberger is a scholar working on Astronomy and Astrophysics, Molecular Biology and Computational Mechanics. According to data from OpenAlex, W. Schaffenberger has authored 13 papers receiving a total of 307 indexed citations (citations by other indexed papers that have themselves been cited), including 9 papers in Astronomy and Astrophysics, 3 papers in Molecular Biology and 2 papers in Computational Mechanics. Recurrent topics in W. Schaffenberger's work include Solar and Space Plasma Dynamics (9 papers), Ionosphere and magnetosphere dynamics (4 papers) and Stellar, planetary, and galactic studies (3 papers). W. Schaffenberger is often cited by papers focused on Solar and Space Plasma Dynamics (9 papers), Ionosphere and magnetosphere dynamics (4 papers) and Stellar, planetary, and galactic studies (3 papers). W. Schaffenberger collaborates with scholars based in United States, Germany and Austria. W. Schaffenberger's co-authors include O. Steiner, B. Freytag, Sven Wedemeyer, M. Steffen, H.‐G. Ludwig, A. Hanslmeier, M. Roth, Н. В. Еркаев, C. J. Farrugia and H. K. Biernat and has published in prestigious journals such as Journal of Computational Physics, Astronomy and Astrophysics and Planetary and Space Science.

In The Last Decade

W. Schaffenberger

12 papers receiving 292 citations

Peers

W. Schaffenberger
C. Damiani France
E. Páez Spain
J. J. Sudol United States
A. Lèbre France
C. G. Toner United States
W. Schaffenberger
Citations per year, relative to W. Schaffenberger W. Schaffenberger (= 1×) peers Veronika Witzke

Countries citing papers authored by W. Schaffenberger

Since Specialization
Citations

This map shows the geographic impact of W. Schaffenberger'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 W. Schaffenberger with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W. Schaffenberger more than expected).

Fields of papers citing papers by W. Schaffenberger

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by W. Schaffenberger. 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 W. Schaffenberger. The network helps show where W. Schaffenberger may publish in the future.

Co-authorship network of co-authors of W. Schaffenberger

This figure shows the co-authorship network connecting the top 25 collaborators of W. Schaffenberger. A scholar is included among the top collaborators of W. Schaffenberger 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 W. Schaffenberger. W. Schaffenberger is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

13 of 13 papers shown
1.
Steiner, O., et al.. (2014). Properties of small-scale magnetism of stellar atmospheres. Publications of the Astronomical Society of Japan. 66(SP1). 9 indexed citations
2.
Steiner, O., et al.. (2011). Modification of wave propagation and wave travel-time by the presence of magnetic fields in the solar network atmosphere. Astronomy and Astrophysics. 538. A79–A79. 16 indexed citations
3.
Freytag, B., M. Steffen, H.‐G. Ludwig, et al.. (2011). Simulations of stellar convection with CO5BOLD. Journal of Computational Physics. 231(3). 919–959. 243 indexed citations
4.
O’Shea, Brian W., et al.. (2010). Tutorials in Introductory Physics: The Pain and the Gain. The Physics Teacher. 48(7). 453–457. 6 indexed citations
5.
Freytag, B., M. Steffen, Sven Wedemeyer, et al.. (2010). CO5BOLD: COnservative COde for the COmputation of COmpressible COnvection in a BOx of L Dimensions with l. Dépôt institutionnel de l'Université libre de Bruxelles (Université Libre de Bruxelles). 11014. 1 indexed citations
6.
Stein, Robert F., et al.. (2007). Solar Magneto-Convection Simulations. Research at the University of Copenhagen (University of Copenhagen). 369. 87.
7.
Stein, Robert F., Dali Georgobiani, Åke Nordlund, et al.. (2007). Surface Convection. AIP conference proceedings. 111–115. 4 indexed citations
8.
Schaffenberger, W., Sven Wedemeyer, O. Steiner, & B. Freytag. (2006). Holistic MHD-Simulation from the Convection Zone to the Chromosphere. 354. 345. 3 indexed citations
9.
Schaffenberger, W., Sven Wedemeyer, O. Steiner, & B. Freytag. (2005). Magnetohydrodynamic Simulation from the Convection Zone to the Chromosphere. 596. 7 indexed citations
10.
Wedemeyer, Sven, W. Schaffenberger, O. Steiner, et al.. (2005). Simulations of Magnetohydrodynamics and CO Formation from the Convection Zone to the Chromosphere. 596. 2 indexed citations
11.
Schaffenberger, W. & A. Hanslmeier. (2002). Two-dimensional lattice Boltzmann model for magnetohydrodynamics. Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics. 66(4). 46702–46702. 8 indexed citations
12.
Еркаев, Н. В., et al.. (2001). Analysis of mirror modes convected from the bow shock to the magnetopause. Planetary and Space Science. 49(13). 1359–1364. 5 indexed citations
13.
Biernat, H. K., et al.. (2000). MHD effects of the solar wind flow around planets. Nonlinear processes in geophysics. 7(3/4). 201–210. 3 indexed citations

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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026