This map shows the geographic impact of W. Schmütz'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. Schmütz with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W. Schmütz more than expected).
This network shows the impact of papers produced by W. Schmütz. 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. Schmütz. The network helps show where W. Schmütz may publish in the future.
Co-authorship network of co-authors of W. Schmütz
This figure shows the co-authorship network connecting the top 25 collaborators of W. Schmütz.
A scholar is included among the top collaborators of W. Schmütz 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. Schmütz. W. Schmütz is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Egorova, Tatiana, W. Schmütz, Eugene Rozanov, et al.. (2018). Revised historical solar irradiance forcing. Springer Link (Chiba Institute of Technology).52 indexed citations
Thuillier, Gérard, A. I. Shapiro, T. N. Woods, et al.. (2015). SOLSPEC investigation on board the International Space Station: The Absolute Solar Spectral Irradiance in the Infrared Domain. EGU General Assembly Conference Abstracts. 9663.1 indexed citations
Shapiro, A. I., W. Schmütz, Gaël Cessateur, & Eugene Rozanov. (2013). The place of the Sun among the Sun-like stars. Springer Link (Chiba Institute of Technology).13 indexed citations
10.
Rozanov, Eugene, A. V. Shapiro, J. W. Harder, et al.. (2011). The stratospheric ozone response to a discrepancy of the SSI data. AGUFM. 2011.
11.
Shapiro, A. I., W. Schmütz, Micha Schoell, Margit Haberreiter, & Eugene Rozanov. (2010). NLTE solar irradiance modeling with the COSI code. Springer Link (Chiba Institute of Technology).52 indexed citations
12.
Hochedez, J.‐F., I. E. Dammasch, & W. Schmütz. (2010). First results from the LYRA solar UV radiometer. 38. 4.1 indexed citations
13.
Thuillier, Gérard, David Bolsée, G. Schmidtke, et al.. (2010). The Absolute Solar Irradiance Spectrum at Solar Minimum Activity Measured by the SOLSPEC and SOL-ACES Spectrometers from 17 to 3000 nm Placed on Board the International Space Station. cosp. 38. 7.
14.
Berghmans, D., J.‐F. Hochedez, A. BenMoussa, et al.. (2005). Space Weather with ESA's PROBA2 Mission. ESASP. 592. 685.1 indexed citations
15.
Haberreiter, Margit, N. A. Krivova, W. Schmütz, & T. Wenzler. (2004). Reconstruction of solar UV irradiance back to 1974. Max Planck Digital Library. 35. 2707.2 indexed citations
16.
Crowther, P. A., L. J. Smith, D. J. Hillier, & W. Schmütz. (1995). Fundamental parameters of Wolf-Rayet stars. III. The evolutionary status of WNL stars.. A&A. 293. 427–445.1 indexed citations
17.
Nussbaumer, H., et al.. (1995). Proof of a fast wind in the symbiotic nova AG Pegasi.. A&A. 293.1 indexed citations
18.
Schmütz, W.. (1993). Analysis of the IR Spectrum of Cygnus X-3. 10. 259.1 indexed citations
19.
Schmütz, W. & William D. Vacca. (1991). Determinations of the interstellar reddening toward Wolf-Rayet stars of the nitrogen sequence from observed UBV color indices.. Astronomy & Astrophysics Supplement Series. 89(2). 259–284.
20.
Hamann, W.‐R., et al.. (1987). Spectral Analysis of the Wolf-Rayet Star HD 50896. 194. 190–196.3 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.