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.
Chromospheric Alfvenic Waves Strong Enough to Power the Solar Wind
2007539 citationsT. D. Tarbell, C. J. Schrijver 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. A. Shine'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. A. Shine with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. A. Shine more than expected).
This network shows the impact of papers produced by R. A. Shine. 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. A. Shine. The network helps show where R. A. Shine may publish in the future.
Co-authorship network of co-authors of R. A. Shine
This figure shows the co-authorship network connecting the top 25 collaborators of R. A. Shine.
A scholar is included among the top collaborators of R. A. Shine 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. A. Shine. R. A. Shine 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.
Shine, R. A., R. W. Nightingale, P. Boerner, T. D. Tarbell, & C. J. Wolfson. (2010). Flat Fielding and Image Alignments for AIA/SDO Data Images. AGU Fall Meeting Abstracts. 2010.2 indexed citations
Brown, D. S., R. W. Nightingale, D. M. Alexander, et al.. (2002). Observations of rotating sunspots and their effect in the corona. ESASP. 505. 261–264.1 indexed citations
Hagenaar, H. J., C. J. Schrijver, R. A. Shine, & A. M. Title. (1997). Dispersal of magnetic flux in the quiet network as observed on a day-long magnetogram sequences observed with MDI on SOHO. 28.1 indexed citations
6.
Simon, Gilles, et al.. (1995). Warning: Local Correlation Tracking may BE Dangerous to your (scientific) Health. ESASP. 376. 223.1 indexed citations
Brandt, Peter, R. J. Rutten, R. A. Shine, & J. Trujillo Bueno. (1992). Dynamics of the Quiet Solar Atmosphere: K2v Cell Grains Versus Magnetic Elements. 26. 161.1 indexed citations
9.
Title, A. M., Z. Frank, R. A. Shine, & T. D. Tarbell. (1991). Field Geometry of Sunspots Inferred from Inclination Effects. Bulletin of the American Astronomical Society. 23. 1052.1 indexed citations
10.
Frank, Z., R. A. Shine, G. L. Slater, T. D. Tarbell, & K. Topka. (1990). Generation of Waves and Electric Currents on Magnetic Flux Tubes by Horizontal and Vertical Velocities in the Photosphere. Bulletin of the American Astronomical Society. 22. 878.7 indexed citations
11.
Shine, R. A., B. E. Woodgate, & J. B. Gurman. (1984). Center-to-Limb Variation of Transition Region Redshift. Bulletin of the American Astronomical Society. 16. 992.1 indexed citations
12.
Woodgate, B. E., R. A. Shine, E. J. Schmahl, M. R. Kundu, & V. Gaizauskas. (1982). Upflows Immediately Prior to the Impulsive Phase of Solar Flares. Bulletin of the American Astronomical Society. 14. 898.2 indexed citations
13.
Gebbie, K. B., F. Hill, Juri Toomre, et al.. (1980). Steady Flows in the Solar Transition Region Observed with the UVSP Experiment on SMM. Bulletin of the American Astronomical Society. 12. 907.1 indexed citations
14.
Shine, R. A. & B. W. Lites. (1977). Center-to-Limb Profiles and Spatial Variations of SiII and FeII Lines in the Solar EUV.. Bulletin of the American Astronomical Society. 9. 325.1 indexed citations
15.
Shine, R. A., E. G. Chipman, E. C. Bruner, et al.. (1976). OSO-8 Observations of Mean Vertical Motions in the Solar Transition Region. Bulletin of the American Astronomical Society. 8. 312.2 indexed citations
16.
Lites, B. W. & R. A. Shine. (1976). Analysis of OSO-8 Measurements of the Center-to-Limb Behavior of Solar CII Line Profiles.. Bulletin of the American Astronomical Society. 8. 501.1 indexed citations
17.
November, L. J., Juri Toomre, K. B. Gebbie, et al.. (1976). Supergranulation Velocity Fields Observed in the Solar Transition Region with OSO-8. Bulletin of the American Astronomical Society. 8. 311.1 indexed citations
18.
Bruner, E. C., E. G. Chipman, B. W. Lites, et al.. (1975). High Resolution Spectroscopy From Orbiting Solar Observatory VIII: Transition Zone Dynamics Over a Sunspot. Bulletin of the American Astronomical Society. 7. 522.
19.
Ayres, T. R., Jeffrey L. Linsky, & R. A. Shine. (1975). Stellar Upper Photosphere Models Based on the Ca II K-wing. II. The Coherent Scattering Approximation. Bulletin of the American Astronomical Society. 7. 359.1 indexed citations
20.
Shine, R. A.. (1974). Non-LTE Line Formation in the Presence of Intermediate Scale Velocity Fields. Bulletin of the American Astronomical Society. 6. 294.1 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.