R. Schwenn
About
In The Last Decade
R. Schwenn
149 papers receiving 7.4k citations
Hit Papers
Peers
Comparison fields: 5 of 66
- Astronomy and Astrophysics 8.0k
- Molecular Biology 2.2k
- Artificial Intelligence 422
- Geophysics 295
- Nuclear and High Energy Physics 294
Countries citing papers authored by R. Schwenn
This map shows the geographic impact of R. Schwenn'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 R. Schwenn with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. Schwenn more than expected).
Fields of papers citing papers by R. Schwenn
This network shows the impact of papers produced by R. Schwenn. 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 R. Schwenn. The network helps show where R. Schwenn may publish in the future.
Co-authorship network of co-authors of R. Schwenn
This figure shows the co-authorship network connecting the top 25 collaborators of R. Schwenn. A scholar is included among the top collaborators of R. Schwenn 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 R. Schwenn. R. Schwenn is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | Forecasting interplanetary ejecta arrival at 1 AU | 2 |
| 2 | Comparison between halo CME expansion speeds observed on the sun, their average propagation speeds to earth and their corresponding counterparts near earth | 2 |
| 3 | Causes of major magnetic storms near the latest solar maximum | 3 |
| 4 | A Tool For Improved Space Weather Predictions: The CME Expansion Speed | 13 |
| 5 | Solar Orbiter --- A High Resolution Mission to the Sun and Inner Heliosphere | 3 |
| 6 | On the rotation rate of the emission solar corona | 2 |
| 7 | European Plans for the Solar/Heliospheric Stereo Mission | 0 |
| 8 | Electronic densities in coronal holes from LASCO-C2 images. | 4 |
| 9 | Dynamical evolution of a coronal mass ejection (CME) to magnetic cloud: A preliminary analysis of the January 6-10, 1997 CME observed by LASCO/SOHO | 4 |
| 10 | The Large Angle Spectroscopic Coronagraph (LASCO): visible light coronal imaging and spectroscopy. | 1 |
| 11 | Spatial structures in high-speed streams as signatures of fine structures in coronal holes. | 66 |
| 12 | Large-scale propagation properties of an interplanetary disturbance in association with a 'halo' coronal mass ejection on 27 November 1979 | 2 |
| 13 | The solar wind | 2 |
| 14 | Report of ESA's topical team on solar and heliospheric physics. | 1 |
| 15 | Data Analysis of Electron Measurements of the Plasma Experiment aboard the Helios Probes | 4 |
| 16 | Associations between coronal mass ejections and interplanetary shocks | 15 |
| 17 | The average solar wind in the inner heliosphere: Structures and slow variations | 67 |
| 18 | Dynamical evolution of interplanetary magnetic fields and flows between 0.3 AU and 8.5 AU: entrainment. | 1 |
| 19 | Solar Cycle Variation of IPS Transients Observed Near Earth | 3 |
| 20 | Acceleration of gt;= 80 keV ions by interplanetary shocks between 0.3-1 AU observed by Helios-1/2: A survey | 1 |
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.