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.
Results from an extensive Einstein stellar survey
1981181 citationsR. Mewe, C. Zwaan et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of R. Mewe'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. Mewe with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. Mewe more than expected).
This network shows the impact of papers produced by R. Mewe. 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. Mewe. The network helps show where R. Mewe may publish in the future.
Co-authorship network of co-authors of R. Mewe
This figure shows the co-authorship network connecting the top 25 collaborators of R. Mewe.
A scholar is included among the top collaborators of R. Mewe 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. Mewe. R. Mewe 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.
Audard, M., et al.. (2003). . UvA-DARE (University of Amsterdam).62 indexed citations
2.
Mewe, R., et al.. (2003). Improved Line Ratio Calculations for He-like Ions. 12. 1123–1128.1 indexed citations
3.
Audard, M., M. Güdel, R. Mewe, et al.. (2002). A Study of the Coronal Plasma in RS CVn binary systems: HR1099 and co.. CERN Bulletin. 277. 65–73.1 indexed citations
Brinkman, A. C., A. J. F. den Boggende, Luc Dubbeldam, et al.. (1996). X-ray spectroscopy with the Reflection Grating Spectrometer on-board of XMM.. 675–676.
7.
Singh, K. P., N. E. White, S. A. Drake, R. Mewe, & J. S. Kaastra. (1995). Algol: A joint analysis of the EUVE and ASCA Spectra. AAS. 187.
8.
Schrijver, C. J., R. Mewe, G. H. J. van den Oord, & J. S. Kaastra. (1995). EUV spectroscopy of cool stars. II. Coronal structure of selected cool stars observed with the EUVE.. A&A. 302. 438.4 indexed citations
9.
Schrijver, C. J., G. H. J. van den Oord, & R. Mewe. (1994). The optical thickness of stellar coronae in the EUV lines.. A&A. 289.2 indexed citations
10.
Kaastra, J. S. & R. Mewe. (1993). X-ray emission from thin plasmas. I - Multiple Auger ionisation and fluorescence processes for Be to Zn. Astronomy & Astrophysics Supplement Series. 97(2). 443–482.22 indexed citations
11.
Oord, G. H. J. van den & R. Mewe. (1989). The X-ray flare and the quiescent emission from Algol as detected by EXOSAT.. A&A. 213. 245–260.6 indexed citations
12.
Mewe, R., J. R. Lemen, & G. H. J. van den Oord. (1986). Calculated X-radiation from optically thin plasmas. VI - Improved calculations for continuum emission and approximation formulae for nonrelativistic average Gaunt actors.. Astronomy & Astrophysics Supplement Series. 65(3). 511–536.41 indexed citations
13.
Lemen, J. R., J. Sylwester, & R. Mewe. (1984). Variation in the Observed Coronal Calcium Abundance for Various X-Ray Flare Plasmas. Bulletin of the American Astronomical Society. 16. 545.
14.
Mewe, R.. (1982). Einstein Observations of Late-Type Stars of Different Calcium-II Activity. Observatory. 102. 109.1 indexed citations
15.
Mewe, R. & E. H. B. M. Gronenschild. (1981). Calculated X-radiation from optically thin plasmas. IV - Atomic data and rate coefficients for spectra in the range 1-270 A.. Astronomy & Astrophysics Supplement Series. 45. 11–52.29 indexed citations
16.
Mewe, R. & C. Zwaan. (1980). Chromospheric and Coronal Activity in F-Type G-Type and K-Type Stars. 389. 123.
17.
Mewe, R., C. J. Schrijver, & J. Sylwester. (1980). Analysis of X-ray line spectra from a transient plasma under solar flare conditions. II - Rate coefficients. III - Diagnostics for measuring electron temperature and density. 40. 323–346.2 indexed citations
18.
Heise, J., R. Mewe, A. C. Brinkman, et al.. (1978). Detection of both soft and hard X-ray emission from SS Cygni with ANS.. A&A. 63.1 indexed citations
19.
Gronenschild, E. H. B. M. & R. Mewe. (1978). Calculated X-radiation from optically thin plasmas. III. Abundance effects on continuum emission.. Astronomy & Astrophysics Supplement Series. 32. 283–305.3 indexed citations
20.
Mewe, R. & C. J. Schrijver. (1978). Heliumlike ion line intensities. III. Results.. Astronomy & Astrophysics Supplement Series. 33. 311–313.6 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.