C. Zwaan
About
In The Last Decade
C. Zwaan
49 papers receiving 2.1k citations
Hit Papers
Peers
Comparison fields: 5 of 68
- Astronomy and Astrophysics 2.1k
- Molecular Biology 473
- Artificial Intelligence 228
- Instrumentation 157
- Oceanography 116
Countries citing papers authored by C. Zwaan
This map shows the geographic impact of C. Zwaan'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 C. Zwaan with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. Zwaan more than expected).
Fields of papers citing papers by C. Zwaan
This network shows the impact of papers produced by C. Zwaan. 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 C. Zwaan. The network helps show where C. Zwaan may publish in the future.
Co-authorship network of co-authors of C. Zwaan
This figure shows the co-authorship network connecting the top 25 collaborators of C. Zwaan. A scholar is included among the top collaborators of C. Zwaan 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 C. Zwaan. C. Zwaan is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 13 | |
| 2 | 6 | |
| 3 | PHENOMENA IN AN EMERGING ACTIVE REGION. I. HORIZONTAL DYNAMICS | 33 |
| 4 | Patterns in the solar magnetic field (Invited Review) | 1 |
| 5 | 3 | |
| 6 | Magnetic structure in cool stars. XVIII : UV-line emissions from T Tauri stars | 1 |
| 7 | Activity in Tidally Interacting Binaries | 3 |
| 8 | Magnetic structure in cool stars. XVI. Emissions from the outer atmospheres of M-type dwarfs | 2 |
| 9 | 28 | |
| 10 | Magnetic structure in cool stars. VIII: The Mg II h and k surface fluxes in relation to the Mt. Wilson photometric Ca II H and K measurements | 4 |
| 11 | Empirical NLTE analyses of solar spectral lines. IV - The Fe I curve of growth | 0 |
| 12 | Large-Scale Patterns in Solar Activity During the Ascending Phase of Cycle 21 | 0 |
| 13 | Magnetic braking in low-mass X-ray binaries. | 12 |
| 14 | 0 | |
| 15 | 10 | |
| 16 | A Polarimeter for a Fourier Transform Spectrometer and Initial Solar Observations | 2 |
| 17 | Chromospheric and Coronal Activity in F-Type G-Type and K-Type Stars | 0 |
| 18 | Methods for the analysis of stellar spectra veiled by lines (III). | 2 |
| 19 | 115 | |
| 20 | 3 |
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.