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.
Modeling the Sun’s Magnetic Field and Irradiance since 1713
2005439 citationsJ. Lean, N. R. Sheeley et al.profile →
Measurements of Flow Speeds in the Corona Between 2 and 30R☉
1997410 citationsN. R. Sheeley, R. A. Howard et al.profile →
Citations per year, relative to N. R. Sheeley N. R. Sheeley (= 1×)
peers
P. H. Scherrer
Countries citing papers authored by N. R. Sheeley
Since
Specialization
Citations
This map shows the geographic impact of N. R. Sheeley'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 N. R. Sheeley with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites N. R. Sheeley more than expected).
This network shows the impact of papers produced by N. R. Sheeley. 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 N. R. Sheeley. The network helps show where N. R. Sheeley may publish in the future.
Co-authorship network of co-authors of N. R. Sheeley
This figure shows the co-authorship network connecting the top 25 collaborators of N. R. Sheeley.
A scholar is included among the top collaborators of N. R. Sheeley 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 N. R. Sheeley. N. R. Sheeley 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.
Sheeley, N. R.. (2009). Remote-sensing Observations of the Corona and Solar Wind. AAS. 214.1 indexed citations
2.
Whang, Y. C., et al.. (2003). The termination shock near 35 degrees latitude. AGU Fall Meeting Abstracts. 2003.1 indexed citations
3.
Lean, J., et al.. (2003). Modeling the Sun's polar fields and open flux during the Maunder Minimum. EGS - AGU - EUG Joint Assembly. 2424.1 indexed citations
4.
Kahler, S. W., D. V. Reames, & N. R. Sheeley. (2001). A CME associated with an impulsive SEP event. ICRC. 8. 3443.6 indexed citations
5.
Sheeley, N. R.. (1992). The Flux-Transport Model and Its Implications. ASPC. 27. 1.1 indexed citations
6.
Kahler, S. W., D. V. Reames, & N. R. Sheeley. (1990). Coronal Mass Ejections and the Injection Profiles of Solar Energetic Particle Events. ICRC. 5. 183.3 indexed citations
7.
Harvey, K. L., N. R. Sheeley, & John G. Harvey. (1986). HE I 10830 A Observations of Two-Ribbon Flare-Like Events Associated with Filament Disappearances. 198.5 indexed citations
8.
Sheeley, N. R., R. A. Howard, & K. L. Harvey. (1984). Coronal Mass Ejections and Sudden Filament Disappearances. Bulletin of the American Astronomical Society. 16. 930.1 indexed citations
9.
Sheeley, N. R., R. A. Howard, M. J. Koomen, et al.. (1983). Associations between coronal mass ejections and interplanetary shocks. MPG.PuRe (Max Planck Society). 228. 693–702.15 indexed citations
10.
Kahler, S. W., N. R. Sheeley, R. A. Howard, et al.. (1983). Associations between Coronal Mass Ejections and Solar Energetic Proton Events. Bulletin of the American Astronomical Society. 15. 699.1 indexed citations
11.
Kahler, S. W., R. E. McGuire, D. V. Reames, et al.. (1983). The correlation of coronal mass ejections with energetic flare proton events. International Cosmic Ray Conference. 4. 6.3 indexed citations
12.
Howard, R. A., N. R. Sheeley, M. J. Koomen, & D. J. Michels. (1983). On the Nature of Coronal Mass Ejections During the Period 28 March 1979 through 30 June 1981. Bulletin of the American Astronomical Society. 15. 703.1 indexed citations
13.
Koomen, M. J., D. J. Michels, R. A. Howard, & N. R. Sheeley. (1980). The Lateral Expansion of the August 14, 1979 Coronal Transient. Bulletin of the American Astronomical Society. 12. 515.1 indexed citations
14.
Sheeley, N. R., R. A. Howard, M. J. Koomen, et al.. (1980). Solar Cycle Variation of IPS Transients Observed Near Earth. Bulletin of the American Astronomical Society. 12. 920.3 indexed citations
15.
Harvey, K. L. & N. R. Sheeley. (1980). Coronal Holes and the Sun's Mean Magnetic Field. Bulletin of the American Astronomical Society. 12. 918.1 indexed citations
16.
Sheeley, N. R., J. D. Bohlin, G. E. Brueckner, et al.. (1975). Interpreting XUV Spectroheliograms in Terms of Coronal Magnetic Field Structures. Bulletin of the American Astronomical Society. 7. 346.2 indexed citations
17.
Bohlin, J. D., J. D. Purcell, N. R. Sheeley, & R. Tousey. (1975). Polar Plumes in XUV Emission-Line Corona. Bulletin of the American Astronomical Society. 7. 356.5 indexed citations
18.
Bohlin, J. D., et al.. (1975). The Sun's Polar Caps as Coronal Holes: Their Sizes, Evolution, and Phenomenology During the Skylab Mission.. Bulletin of the American Astronomical Society. 7. 457.5 indexed citations
19.
Bohlin, J. D., G. E. Brueckner, J. D. Purcell, et al.. (1974). The eruptive prominence of August 21, 1973 observed from Skylab in the white light corona and in the He II 304 Å chromosphere.. Bulletin of the American Astronomical Society. 6. 219.2 indexed citations
20.
Allen, Richard D., et al.. (1973). Magnetic Outflow - A Stage in the Development of an Active Region. Bulletin of the American Astronomical Society. 5. 268.2 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.