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.
Velocity Fields in the Solar Atmosphere. I. Preliminary Report.
1962449 citationsRobert B. Leighton, R. W. Noyes et al.The Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
Countries citing papers authored by George W. Simon
Since
Specialization
Citations
This map shows the geographic impact of George W. Simon'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 George W. Simon with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites George W. Simon more than expected).
This network shows the impact of papers produced by George W. Simon. 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 George W. Simon. The network helps show where George W. Simon may publish in the future.
Co-authorship network of co-authors of George W. Simon
This figure shows the co-authorship network connecting the top 25 collaborators of George W. Simon.
A scholar is included among the top collaborators of George W. Simon 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 George W. Simon. George W. Simon 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.
Strous, Louis H. & George W. Simon. (1998). 62 Days Around the Sun: A Search for Supergranular Evolution and Giant Cells. 140. 161.
2.
Sobotka, M., Peter Brandt, & George W. Simon. (1997). Fine structure in sunspots. II. Intensity variations and proper motions of umbral dots. 328(2). 689–694.6 indexed citations
3.
Sobotka, M., Peter Brandt, & George W. Simon. (1997). Fine structure in sunspots. I. Sizes and lifetimes of umbral dots. FreiDok plus (Universitätsbibliothek Freiburg). 328(2). 682–688.16 indexed citations
4.
Balasubramaniam, Krishnan & George W. Simon. (1994). Solar active region evolution: comparing models with observations. ASPC. 68.70 indexed citations
5.
Balasubramaniam, Krishnan & George W. Simon. (1994). Solar active region evolution : comparing models with observations : proceedings of Fourteenth International Summer Workshop National Solar Observatory/Sacramento Peak, Sunspot, New Mexico 88349, USA, 30 August - 3 September 1993. Astronomical Society of the Pacific eBooks.1 indexed citations
Labonte, B. J., George W. Simon, & R. B. Dunn. (1974). A Phenomenological Study of High-Resolution Granulation Photographs. Bulletin of the American Astronomical Society. 6. 285.1 indexed citations
12.
Simon, George W., P. Seagraves, R. Tousey, & R. W. Noyes. (1974). Rocket Spectroheliogram Observations of the Heights of Formation and Sizes of Bright Features in the Transition Zone. Bulletin of the American Astronomical Society. 6. 294.1 indexed citations
Simon, George W. & R. W. Noyes. (1971). Observations of the Coronal Network. Symposium - International Astronomical Union. 43. 663–666.9 indexed citations
Leighton, Robert B., R. W. Noyes, & George W. Simon. (1962). Velocity Fields in the Solar Atmosphere. I. Preliminary Report.. The Astrophysical Journal. 135. 474–474.449 indexed citations breakdown →
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.