This map shows the geographic impact of O. Steiner'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 O. Steiner with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites O. Steiner more than expected).
This network shows the impact of papers produced by O. Steiner. 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 O. Steiner. The network helps show where O. Steiner may publish in the future.
Co-authorship network of co-authors of O. Steiner
This figure shows the co-authorship network connecting the top 25 collaborators of O. Steiner.
A scholar is included among the top collaborators of O. Steiner 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 O. Steiner. O. Steiner is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
20 of 20 papers shown
1.
Steiner, O., et al.. (2017). CO5BOLD for MHD: progresses and deficiencies .. MmSAI. 88. 37.1 indexed citations
Steiner, O. & R. Rezaei. (2012). Recent Advances in the Exploration of the Small-Scale Structure of the Quiet Solar Atmosphere: Vortex Flows, the Horizontal Magnetic Field, and the Stokes- V Line-Ratio Method. 456. 3.4 indexed citations
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
7.
Schaffenberger, W., Sven Wedemeyer, O. Steiner, & B. Freytag. (2005). Magnetohydrodynamic Simulation from the Convection Zone to the Chromosphere. 596.7 indexed citations
8.
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
Steiner, O.. (2001). The Formation of Asymmetric Stokes V Profiles in the Presence of a Magnetopause. FreiDok plus (Universitätsbibliothek Freiburg). 236. 587.2 indexed citations
12.
Leka, K. D., O. Steiner, & U. Grossmann‐Doerth. (1999). Understanding Small Solar Magnetic Elements: Comparing Models and Observations. 194.
13.
Grossmann‐Doerth, U., M. Schuessler, & O. Steiner. (1998). Convective intensification of solar surface magnetic fields: results of numerical experiments. FreiDok plus (Universitätsbibliothek Freiburg). 337(3). 928–939.16 indexed citations
14.
Steiner, O.. (1996). Convective intensification of magnetic fields at the solar surface.. 1996(4). 185–192.1 indexed citations
15.
Steiner, O., et al.. (1993). On the interchange instability of solar magnetic flux tubes. I - The influence of magnetic tension and internal gas pressure. 268(1). 299–308.5 indexed citations
16.
Solanki, S. K., et al.. (1991). Two-dimensional models of the solar chromosphere. I - The CA II K line as a diagnostic: 1.5-D radiative transfer. 250(1). 220–234.9 indexed citations
Keller, Christoph U., O. Steiner, J. O. Stenflo, & S. K. Solanki. (1990). Structure of solar magnetic fluxtubes from the inversion of Stokes spectra at disk center. 233(2). 583–597.11 indexed citations
19.
Steiner, O. & V. J. Pizzo. (1989). A parametric survey of model solar fluxtubes. 211(2). 447–462.8 indexed citations
20.
Steiner, O., G. W. Pneuman, & J. O. Stenflo. (1986). Numerical models for solar magnetic fluxtubes. 170(1). 126–137.12 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.