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.
Initial Calibration of the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)
2011289 citationsJ. R. Lemen, C. J. Schrijver et al.profile →
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. 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. 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. Shine more than expected).
This network shows the impact of papers produced by R. 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. Shine. The network helps show where R. Shine may publish in the future.
Co-authorship network of co-authors of R. Shine
This figure shows the co-authorship network connecting the top 25 collaborators of R. Shine.
A scholar is included among the top collaborators of R. 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. Shine. R. Shine is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Lites, B. W., Masahito Kubo, H. Socas‐Navarro, et al.. (2008). Magnetic Fields of the Quiet Sun: A New Quantitative Perspective From Hinode. 397(6). 17–140.1 indexed citations
6.
Katsukawa, Yukio, S. Tsuneta, Y. Suematsu, et al.. (2007). Chromospheric Micro-jets Discovered Above Sunspot Penumbrae. AAS. 210.1 indexed citations
7.
Ichimoto, Kiyoshi, Y. Suematsu, S. Tsuneta, et al.. (2007). Hinode/SOT Observation of Fine Structure of the Evershed Flow. 210.1 indexed citations
8.
Suematsu, Y., Yukio Katsukawa, Kiyoshi Ichimoto, et al.. (2007). High Resolution Observation of Spicules in Ca II H with Hinode/SOT. AAS. 210.1 indexed citations
9.
Alford, Ross A., Lin Schwarzkopf, Gregory P. Brown, Ben L. Phillips, & R. Shine. (2006). Characteristics of Bufo marinus in old and recently established populations. ResearchOnline at James Cook University (James Cook University).5 indexed citations
Hurlburt, N. E., S. Freeland, R. Shine, & Prosenjit Bose. (2001). A Prototype Problem-Solving Environment for Living With a Star Data. AGU Fall Meeting Abstracts. 2001.1 indexed citations
Wolfson, Jack M., J. R. Lemen, C. J. Schrijver, et al.. (1997). The TRACE Mission. 28.
17.
Shine, R., T. D. Tarbell, A. M. Title, et al.. (1989). Observations of Running Penumbral Waves. Bulletin of the American Astronomical Society. 21. 837.1 indexed citations
18.
Wolfson, J. L., S. H. Ferguson, Z. Frank, et al.. (1988). Solar Activity and Flare Observations from the Swedish Solar Observatory on La Palma. Bulletin of the American Astronomical Society. 20. 978.1 indexed citations
Shine, R. & Ludwig Oster. (1973). The Effect of Small and Large Scale Sine Waves upon Chromospheric Line Profiles. Bulletin of the American Astronomical Society. 5. 279.1 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.