Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
The Large Angle Spectroscopic Coronagraph (LASCO)
19951.9k citationsG. E. Brueckner, R. A. Howard et al.Solar Physicsprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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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).
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
20 of 20 papers shown
1.
Schwenn, R., A. Dal Lago, E. Huttunen, & W. D. González. (2004). The association of CMEs their counterparts near the Earth. cosp. 35. 2634.2 indexed citations
2.
Kaufmann, P., C. G. Giménez de Castro, В. С. Махмутов, et al.. (2003). The launch of solar coronal mass ejections and submillimeter pulse bursts. MPG.PuRe (Max Planck Society). 23. 24–24.1 indexed citations
Sheeley, N. R., G. E. Brueckner, R. A. Howard, et al.. (1997). Using LASCO Observations to Infer Solar Wind Flow Near the Sun.3 indexed citations
7.
Schwenn, R., et al.. (1995). Statistical analysis of interplanetary shock waves observed during a complete solar activity cycle. NASA Technical Reports Server (NASA). 99.2 indexed citations
8.
Brueckner, G. E., R. A. Howard, M. J. Koomen, et al.. (1995). The Large Angle Spectroscopic Coronagraph (LASCO). Solar Physics. 162(1-2). 357–402.1943 indexed citations breakdown →
9.
Schwenn, R., E. Marsch, & B. V. Jackson. (1993). Book-Review - Physics of the Inner Heliosphere - Part Two - Particles Waves and Turbulence. Solar Physics. 145. 405.3 indexed citations
10.
Marsch, E., et al.. (1992). Solar wind seven : proceedings of the 3rd COSPAR Colloquium held in Goslar, Germany, 16-20 September 1991. Pergamon Press eBooks.2 indexed citations
11.
Marsch, E. & R. Schwenn. (1992). Solar Wind Seven; Proceedings of the 3rd COSPAR Colloquium, Goslar, Germany, Sept. 16-20, 1991.4 indexed citations
12.
Schwenn, R. & E. Marsch. (1991). Particles, waves and turbulence. Springer eBooks.8 indexed citations
13.
Schwenn, R. & E. Marsch. (1990). Large-scale phenomena. Springer eBooks.6 indexed citations
14.
Schwenn, R. & H. Rosenbauer. (1984). Ten years solar wind experiments on HELIOS 1 and HELIOS 2. Geochimica et Cosmochimica Acta Supplement. 66.
15.
Gurnett, D. A., et al.. (1981). Correlation of solar radio bursts associated with electron plasma oscillations, solar particles and shock waves. International Cosmic Ray Conference. 10. 1–4.1 indexed citations
16.
Rosenbauer, H., et al.. (1981). The instruments of the plasma experiment onboard the HELIOS solar probe.2 indexed citations
17.
Schwenn, R., K.‐H. Mühlhäuser, E. Marsch, & H. Rosenbauer. (1981). Two states of the solar wind at the time of solar activity minimum - II. Radial gradients of plasma parameters in fast and slow streams. MPG.PuRe (Max Planck Society). 126–130.26 indexed citations
18.
Pilipp, W., R. Schwenn, E. Marsch, K.‐H. Mühlhäuser, & H. Rosenbauer. (1981). Electron characteristics in the solar wind as deduced from Helios observations. MPG.PuRe (Max Planck Society). 241–249.20 indexed citations
19.
Schwenn, R., K.‐H. Mühlhäuser, & H. Rosenbauer. (1981). Two states of the solar wind at the time of solar activity minimum - I. Boundary layers between fast and slow streams. MPG.PuRe (Max Planck Society). 118–125.10 indexed citations
20.
Gurnett, D. A., F. M. Neubauer, & R. Schwenn. (1979). Plasma wave turbulence associated with an interplanetary shock. [wave in solar wind upstream of magnetosphere]. NASA Technical Reports Server (NASA).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.