J. Feynman

3.9k total citations
83 papers, 2.9k citations indexed

About

J. Feynman is a scholar working on Astronomy and Astrophysics, Molecular Biology and Atmospheric Science. According to data from OpenAlex, J. Feynman has authored 83 papers receiving a total of 2.9k indexed citations (citations by other indexed papers that have themselves been cited), including 70 papers in Astronomy and Astrophysics, 30 papers in Molecular Biology and 7 papers in Atmospheric Science. Recurrent topics in J. Feynman's work include Solar and Space Plasma Dynamics (65 papers), Geomagnetism and Paleomagnetism Studies (30 papers) and Ionosphere and magnetosphere dynamics (29 papers). J. Feynman is often cited by papers focused on Solar and Space Plasma Dynamics (65 papers), Geomagnetism and Paleomagnetism Studies (30 papers) and Ionosphere and magnetosphere dynamics (29 papers). J. Feynman collaborates with scholars based in United States, United Kingdom and Germany. J. Feynman's co-authors include A. Ruzmaikin, Stephen Gabriel, S. F. Martin, N. U. Crooker, E. W. Cliver, S. Gabriel, S. M. Silverman, D. A. Hardy, T. E. Moore and R. L. Arnoldy and has published in prestigious journals such as Nature, Journal of Geophysical Research Atmospheres and The Astrophysical Journal.

In The Last Decade

J. Feynman

80 papers receiving 2.5k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
J. Feynman United States 29 2.4k 893 397 306 222 83 2.9k
K. Kudela Slovakia 29 2.7k 1.1× 644 0.7× 357 0.9× 115 0.4× 452 2.0× 274 3.0k
M. J. Owens United Kingdom 42 4.8k 2.0× 2.0k 2.2× 478 1.2× 282 0.9× 225 1.0× 228 5.2k
M. Storini Italy 25 1.9k 0.8× 435 0.5× 411 1.0× 79 0.3× 133 0.6× 152 2.2k
Mike Hapgood United Kingdom 27 2.2k 0.9× 776 0.9× 377 0.9× 94 0.3× 451 2.0× 90 2.5k
H. Mavromichalaki Greece 28 2.2k 0.9× 397 0.4× 402 1.0× 59 0.2× 343 1.5× 188 2.6k
David H. Hathaway United States 31 3.6k 1.5× 975 1.1× 355 0.9× 288 0.9× 67 0.3× 106 4.0k
W. Kent Tobiska United States 32 4.7k 1.9× 782 0.9× 1.5k 3.7× 194 0.6× 354 1.6× 151 5.1k
D. F. Smart United States 35 3.7k 1.5× 801 0.9× 634 1.6× 148 0.5× 365 1.6× 245 4.7k
H. V. Cane United States 48 7.5k 3.1× 1.8k 2.0× 431 1.1× 60 0.2× 356 1.6× 146 7.6k
W. D. Pesnell United States 24 3.8k 1.6× 662 0.7× 480 1.2× 155 0.5× 138 0.6× 93 4.0k

Countries citing papers authored by J. Feynman

Since Specialization
Citations

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

Fields of papers citing papers by J. Feynman

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by J. Feynman. 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 J. Feynman. The network helps show where J. Feynman may publish in the future.

Co-authorship network of co-authors of J. Feynman

This figure shows the co-authorship network connecting the top 25 collaborators of J. Feynman. A scholar is included among the top collaborators of J. Feynman 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 J. Feynman. J. Feynman 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.
Wang, Jingxiu, et al.. (2011). Statistical properties of superactive regions during solar cycles 19–23. Astronomy and Astrophysics. 534. A47–A47. 37 indexed citations
2.
Ruzmaikin, A., J. Feynman, & Stilian Stoev. (2011). Distribution and clustering of fast coronal mass ejections. Journal of Geophysical Research Atmospheres. 116(A4). n/a–n/a. 10 indexed citations
3.
Jun, Insoo, et al.. (2006). Statistics of solar energetic particle events: Fluences, durations, and time intervals. Advances in Space Research. 40(3). 304–312. 21 indexed citations
4.
Ruzmaikin, A., J. Feynman, Xun Jiang, & Yuk L. Yung. (2005). Extratropical signature of the quasi‐biennial oscillation. Journal of Geophysical Research Atmospheres. 110(D11). 59 indexed citations
5.
Feynman, J., A. Ruzmaikin, & Victor L. Berdichevsky. (2002). The JPL proton fluence model: an update. Journal of Atmospheric and Solar-Terrestrial Physics. 64(16). 1679–1686. 48 indexed citations
6.
Ruzmaikin, A., J. Feynman, M. Neugebauer, & E. J. Smith. (2000). On the Nature and Persistence of Preferred Longitudes of Solar Activity.. 31. 2 indexed citations
7.
Neugebauer, M., E. J. Smith, A. Ruzmaikin, J. Feynman, & A. H. Vaughan. (2000). The solar magnetic field and the solar wind: Existence of preferred longitudes. Journal of Geophysical Research Atmospheres. 105(A2). 2315–2324. 57 indexed citations
8.
Feynman, J. & A. Ruzmaikin. (1999). Problems in the forecasting of solar particle events for manned missions. Radiation Measurements. 30(3). 275–280. 12 indexed citations
9.
Feynman, J.. (1995). Coronal Mass Ejections and Solar Proton Events During the Great March 1989 Disturbances. NASA Technical Reports Server (NASA). 1 indexed citations
10.
Feynman, J. & S. F. Martin. (1995). The initiation of coronal mass ejections by newly emerging magnetic flux. Journal of Geophysical Research Atmospheres. 100(A3). 3355–3367. 207 indexed citations
11.
Feynman, J. & A. Ruzmaikin. (1994). Distributions of the interplanetary magnetic field revisited. Journal of Geophysical Research Atmospheres. 99(A9). 17645–17651. 33 indexed citations
12.
Feynman, J., et al.. (1993). Interplanetary proton fluence model: JPL 1991. Journal of Geophysical Research Atmospheres. 98(A8). 13281–13294. 218 indexed citations
13.
Ruzmaikin, A., et al.. (1992). On Long-Term Dynamics of the Solar Cycle. 27. 547. 4 indexed citations
14.
Feynman, J. & Henry B. Garrett. (1987). Solar Cycle Dependence of Major Equatorial Coronal Mass Ejection Occurrence Rate (from proxy data). 2. 279. 3 indexed citations
15.
Christon, S. P., J. Feynman, & J. A. Slavin. (1987). Dynamic substorm injections - Similar magnetospheric phenomena at earth and Mercury. NASA Technical Reports Server (NASA). 393–400. 14 indexed citations
16.
Feynman, J.. (1983). Solar wind variations in the 60-100 year period range: A review. NASA Technical Reports Server (NASA). 228. 3 indexed citations
17.
Feynman, J.. (1982). Geomagnetic and solar wind cycles, 1900–1975. Journal of Geophysical Research Atmospheres. 87(A8). 6153–6162. 165 indexed citations
18.
Feynman, J. & S. M. Silverman. (1980). Auroral changes during the eighteenth and nineteenth centuries and their implications for the solar wind and the long‐term variation of sunspot activity. Journal of Geophysical Research Atmospheres. 85(A6). 2991–2997. 25 indexed citations
19.
Saflekos, N. A., M. F. Tautz, A. G. Rubin, et al.. (1980). Three-dimensional analysis of charging events on days 87 and 114, 1979, from SCATHA. NASA Technical Reports Server (NASA). 1 indexed citations
20.
Crooker, N. U., J. Feynman, & J. T. Gosling. (1977). On the high correlation between long-term averages of solar wind speed and geomagnetic activity. Journal of Geophysical Research Atmospheres. 82(13). 1933–1937. 144 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.

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