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 Solar Oscillations Investigation - Michelson Doppler Imager
19951.6k citationsT. D. Tarbell, A. M. Title et al.Solar Physicsprofile →
Initial Calibration of the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)
2011289 citationsP. Boerner, J. R. Lemen et al.Solar Physicsprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of C. J. Wolfson'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 C. J. Wolfson with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. J. Wolfson more than expected).
This network shows the impact of papers produced by C. J. Wolfson. 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 C. J. Wolfson. The network helps show where C. J. Wolfson may publish in the future.
Co-authorship network of co-authors of C. J. Wolfson
This figure shows the co-authorship network connecting the top 25 collaborators of C. J. Wolfson.
A scholar is included among the top collaborators of C. J. Wolfson 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 C. J. Wolfson. C. J. Wolfson 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, Richard A., C. J. Wolfson, P. Boerner, T. D. Tarbell, & R. W. Nightingale. (2011). Monitoring Image Alignments and Flat Fields for AIA/SDO Data Images. 42.2 indexed citations
2.
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
3.
Cheimets, Peter, D. Caldwell, Cathy Chou, et al.. (2009). SDO-AIA telescope design. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE.12 indexed citations
4.
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
5.
Wülser, J. P., J. R. Lemen, T. D. Tarbell, et al.. (2000). The STEREO-SECCHI extreme ultraviolet imager.. Bulletin of the American Astronomical Society. 32(2). 827.2 indexed citations
Tarbell, T. D., et al.. (1987). The Correlation Tracker Image Stabilization System for HRSO. Bulletin of the American Astronomical Society. 19. 929.5 indexed citations
Leibacher, J. W., K. J. H. Phillips, & C. J. Wolfson. (1981). SMM Observations of Soft X-Ray Line Spectra. Bulletin of the American Astronomical Society. 13. 555.
12.
Strong, K. T., B. R. Dennis, J. W. Leibacher, & C. J. Wolfson. (1981). The Significance of Multiple Flares. Bulletin of the American Astronomical Society. 13. 820.
Wolfson, C. J., L. W. Acton, & J. W. Leibacher. (1978). Soft X-Ray Observations during the Preflare Phase of the Solar Flare Phenomenon.. Bulletin of the American Astronomical Society. 10. 456.4 indexed citations
16.
Avery, L. W., P. A. Feldman, V. Gaizauskas, J. R. Roy, & C. J. Wolfson. (1977). A search for microwave emission from solar X-ray bright point flares.. NASA Technical Reports Server (NASA). 56(3). 327–331.2 indexed citations
17.
Wolfson, C. J., et al.. (1976). The Early Evolution of X-Ray Producing Active Regions. Bulletin of the American Astronomical Society. 8. 317.1 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.