W. Schmidt

11.8k total citations · 2 hit papers
265 papers, 6.7k citations indexed

About

W. Schmidt is a scholar working on Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics and Nuclear and High Energy Physics. According to data from OpenAlex, W. Schmidt has authored 265 papers receiving a total of 6.7k indexed citations (citations by other indexed papers that have themselves been cited), including 179 papers in Astronomy and Astrophysics, 49 papers in Atomic and Molecular Physics, and Optics and 47 papers in Nuclear and High Energy Physics. Recurrent topics in W. Schmidt's work include Solar and Space Plasma Dynamics (120 papers), Stellar, planetary, and galactic studies (71 papers) and Astro and Planetary Science (50 papers). W. Schmidt is often cited by papers focused on Solar and Space Plasma Dynamics (120 papers), Stellar, planetary, and galactic studies (71 papers) and Astro and Planetary Science (50 papers). W. Schmidt collaborates with scholars based in Germany, United States and Spain. W. Schmidt's co-authors include J. C. Niemeyer, Christoph Federrath, Ralf S. Klessen, D. R. G. Schleicher, Mordecai‐Mark Mac Low, Julia Román-Duval, Muhammad Latif, W. Hillebrandt, S. K. Solanki and C. Beck and has published in prestigious journals such as Nature, Physical Review Letters and The Journal of Chemical Physics.

In The Last Decade

W. Schmidt

255 papers receiving 6.4k citations

Hit Papers

An excess of cosmic ray e... 2008 2026 2014 2020 2008 2010 200 400 600

Author Peers

Peers are selected by citation overlap in the author's most active subfields. citations · hero ref

Author Last Decade Papers Cites
W. Schmidt 5.1k 1.6k 752 393 393 265 6.7k
J. C. Raymond 12.7k 2.5× 4.0k 2.5× 845 1.1× 678 1.7× 265 0.7× 459 13.4k
George B. Field 5.2k 1.0× 2.6k 1.6× 773 1.0× 713 1.8× 179 0.5× 100 6.2k
F. P. Keenan 4.1k 0.8× 441 0.3× 2.2k 2.9× 458 1.2× 109 0.3× 420 5.9k
Ellen G. Zweibel 5.0k 1.0× 2.0k 1.2× 290 0.4× 547 1.4× 182 0.5× 193 5.3k
Eric D. Feigelson 10.6k 2.1× 2.2k 1.4× 486 0.6× 97 0.2× 230 0.6× 226 11.4k
D. Lynden–Bell 12.1k 2.4× 2.4k 1.5× 747 1.0× 270 0.7× 399 1.0× 189 13.8k
S. R. Kulkarni 15.2k 3.0× 3.8k 2.4× 936 1.2× 109 0.3× 395 1.0× 449 16.4k
Lyman Spitzer 4.9k 1.0× 1.9k 1.2× 1.6k 2.1× 187 0.5× 358 0.9× 61 7.2k
A. H. Gabriel 3.5k 0.7× 794 0.5× 2.5k 3.3× 367 0.9× 88 0.2× 136 5.9k
Philip R. Goode 4.1k 0.8× 362 0.2× 543 0.7× 747 1.9× 86 0.2× 190 4.8k

Countries citing papers authored by W. Schmidt

Since Specialization
Citations

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

Fields of papers citing papers by W. Schmidt

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of W. Schmidt. A scholar is included among the top collaborators of W. Schmidt 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. Schmidt. W. Schmidt 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.
Domínguez-Fernández, Paola, Xiaolong Du, W. Schmidt, et al.. (2023). Inflationary and Phase-transitional Primordial Magnetic Fields in Galaxy Clusters. The Astrophysical Journal. 944(1). 100–100. 3 indexed citations
2.
Domínguez-Fernández, Paola, Xiaolong Du, Axel Brandenburg, et al.. (2022). Evolution of Primordial Magnetic Fields during Large-scale Structure Formation. The Astrophysical Journal. 929(2). 127–127. 25 indexed citations
3.
Fischer, Catherine, et al.. (2021). Newly formed downflow lanes in exploding granules in the solar photosphere. Springer Link (Chiba Institute of Technology). 2 indexed citations
4.
Cameron, R. H., S. K. Solanki, T. L. Riethmüller, et al.. (2020). Power spectrum of turbulent convection in the solar photosphere. Springer Link (Chiba Institute of Technology). 7 indexed citations
5.
Schmidt, W., et al.. (2017). LARS: An Absolute Reference Spectrograph for solar observations Upgrade from a prototype to a turn-key system. MPG.PuRe (Max Planck Society). 5 indexed citations
6.
Rimmelé, Thomas, Tom Berger, J. P. McMullin, et al.. (2014). The Daniel K. Inouye Solar Telescope: A Project Update.. amos.
7.
Tremblin, Pascal, E. Audit, V. Minier, W. Schmidt, & N. Schneider. (2012). Three-dimensional simulations of globule and pillar formation around HII regions: turbulence and shock curvature. Springer Link (Chiba Institute of Technology). 58 indexed citations
8.
Schmidt, W., et al.. (2010). Numerical and semi-analytic core mass distributions in supersonic isothermal turbulence. Springer Link (Chiba Institute of Technology). 18 indexed citations
9.
Federrath, Christoph, Julia Román-Duval, Ralf S. Klessen, W. Schmidt, & Mordecai‐Mark Mac Low. (2010). Comparing the statistics of interstellar turbulence in simulations and observations. Astronomy and Astrophysics. 512. A81–A81. 549 indexed citations breakdown →
10.
Schmidt, W.. (2007). On the applicability of the level set method beyond the flamelet regime in thermonuclear supernova simulations. Springer Link (Chiba Institute of Technology). 3 indexed citations
11.
Rezaei, R., R. Schlichenmaier, W. Schmidt, & O. Steiner. (2007). Opposite magnetic polarity of two photospheric lines in single spectrum of the quiet Sun. Springer Link (Chiba Institute of Technology). 8 indexed citations
12.
Rezaei, R., O. Steiner, Sven Wedemeyer, et al.. (2007). Hinode observations reveal boundary layers of magnetic elements \n in the solar photosphere. Springer Link (Chiba Institute of Technology). 18 indexed citations
13.
Beck, C., W. Schmidt, R. Rezaei, & W. Rammacher. (2007). The signature of chromospheric heating in Ca II H spectra. Springer Link (Chiba Institute of Technology). 31 indexed citations
14.
Schmidt, W. & J. C. Niemeyer. (2006). Thermonuclear supernova simulations with stochastic ignition. Springer Link (Chiba Institute of Technology). 17 indexed citations
15.
Schlichenmaier, R. & W. Schmidt. (2001). Small-Scale Flow Field in a Sunspot Penumbra. ASPC. 12. 289. 1 indexed citations
16.
Schmidt, W., J. Chang, O. Ganel, et al.. (1999). On the identification of high energy cosmic ray electrons in the Advanced Thin Ionization Calorimeter (ATIC). MPG.PuRe (Max Planck Society). 5. 41–44.
17.
Schmidt, W. & T. Kentischer. (1995). Optical system of an Advanced Solar Correlation Tracker.. Astronomy & Astrophysics Supplement Series. 113. 363. 2 indexed citations
18.
Balthasar, H. & W. Schmidt. (1994). Polarimetry and spectroscopy of a simple sunspot. IV. Umbral structures observed in FeI 1027nm. A&A. 290. 649–654. 1 indexed citations
19.
Schmidt, W. & M. Stix. (1983). Two comments of the sun's differential rotation. A&A. 118(1). 1–3. 1 indexed citations
20.
Schmidt, W., H. Rosenbauer, J. Geiss, & E. G. Shelley. (1981). Heavy Ions in the Solar Wind - First ISEE-1 Results on Temperatures. 450. 1 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