Scott E. Forbush

2.8k citations
31 papers · 974 indexed · h-index 15
Topics
Solar and Space Plasma Dynamics (23 papers)Ionosphere and magnetosphere dynamics (13 papers)Astrophysics and Cosmic Phenomena (7 papers)
Partner nations
United States

In The Last Decade

Scott E. Forbush

29 papers receiving 744 citations

Peers

Scott E. Forbush
Comparison fields: 5 of 49
  • Astronomy and Astrophysics 853
  • Nuclear and High Energy Physics 202
  • Molecular Biology 193
  • Artificial Intelligence 161
  • Atmospheric Science 157
Replace K. G. McCracken with:
K. G. McCracken United States
Miranda Parisi Italy
R. W. Kreplin United States
D. Venkatesan Canada
P. H. Stoker South Africa
R. E. McGuire United States
Leverett Davis United States
K.‐P. Wenzel Netherlands
G. Wibberenz Germany
M. Storini Italy
Scott E. Forbush relative to K. G. McCracken United States K. G. McCracken's profile →
Citations per field
00.5×1.5×
K. G. McCracken · 1×
Citations per year

Countries citing papers authored by Scott E. Forbush

Since Specialization
Citations

This map shows the geographic impact of Scott E. Forbush'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 Scott E. Forbush with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Scott E. Forbush more than expected).

Fields of papers citing papers by Scott E. Forbush

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Scott E. Forbush. 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 Scott E. Forbush. The network helps show where Scott E. Forbush may publish in the future.

Co-authorship network of co-authors of Scott E. Forbush

This figure shows the co-authorship network connecting the top 25 collaborators of Scott E. Forbush. A scholar is included among the top collaborators of Scott E. Forbush 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 Scott E. Forbush. Scott E. Forbush 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
#WorkIndexed citations
1 21
2 20
3
Cosmic-ray diurnal anisotropy 1937 to 1977.5
5
4 23
5 14
6 51
7 20
8 30
9 52
10 21
11 12
12 8
13 1
14 172
15
World-Wide Variations of Cosmic-Ray Intensity
1
16 1
17 9
18 8
19 0
20 19

About Scott E. Forbush

Scott E. Forbush is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Oceanography, having authored 31 papers that have together received 974 indexed citations. Recurring topics across this work include Solar and Space Plasma Dynamics (23 papers), Ionosphere and magnetosphere dynamics (13 papers) and Astrophysics and Cosmic Phenomena (7 papers). The work is most often cited by research in Astronomy and Astrophysics (853 citations), Nuclear and High Energy Physics (202 citations) and Geophysics (117 citations). Scott E. Forbush has collaborated with scholars based in United States. Frequent co-authors include D. Venkatesan, S. P. Duggal, E. H. Vestine, M. A. Pomerantz, John W. Graham, G. Pizzella, H. V. Neher, C. H. Tsao, C. E. McIlwain and B. F. Burke. Their work appears in journals such as Nature, Proceedings of the National Academy of Sciences and Physical Review Letters.

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.

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