T. G. Forbes
- Astronomy and Astrophysics top 1%
- Solar and Space Plasma Dynamics 18
- Ionosphere and magnetosphere dynamics 13
- Astro and Planetary Science 9
- Stellar, planetary, and galactic studies 3
- Gamma-ray bursts and supernovae 1
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- Geomagnetism and Paleomagnetism Studies 5
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- Magnetic confinement fusion research 2
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- Solar Radiation and Photovoltaics 1
T. G. Forbes
19 papers receiving 1.5k citations
Hit Papers
Peers
Comparison fields: 5 of 39
- Astronomy and Astrophysics 1.6k
- Molecular Biology 420
- Nuclear and High Energy Physics 77
- Oceanography 21
- Artificial Intelligence 54
Countries citing papers authored by T. G. Forbes
This map shows the geographic impact of T. G. Forbes'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 T. G. Forbes with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. G. Forbes more than expected).
Fields of papers citing papers by T. G. Forbes
This network shows the impact of papers produced by T. G. Forbes. 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 T. G. Forbes. The network helps show where T. G. Forbes may publish in the future.
Co-authorship network
The 25 scholars most cited alongside T. G. Forbes, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.
All Works
| # | Work | ||
|---|---|---|---|
| 1 | 2024 | 3 | |
| 2 | 2014 | 56 | |
| 3 | 2009 | 34 | |
| 4 | 2007 | 2 | |
| 5 | 2007 | 69 | |
| 6 | 2004 | 1 | |
| 7 | Pre-Eruptive and Eruptive Magnetic Structures in the Solar Corona | 2003 | 2 |
| 8 | 2003 | 7 | |
| 9 | Numerical Test of a Three-Dimensional Flux Rope Model for Coronal Mass Ejections Based on Ideal MHD Processes | 2002 | 1 |
| 10 | Observational Evidence of New Current Sheets Following CMEs | 2001 | 1 |
| 11 | 2001 | 87 | |
| 12 | 2000 | 469 | |
| 13 | Effects of reconnection on the coronal mass ejection processbreakdown → | 2000 | 485 |
| 14 | 1998 | 132 | |
| 15 | 1994 | 38 | |
| 16 | 1990 | 117 | |
| 17 | 1988 | 31 | |
| 18 | A reconnection mechanism for coronal condensations in two-ribbon flares | 1986 | 2 |
| 19 | 1984 | 5 | |
| 20 | 1984 | 0 |
About T. G. Forbes
T. G. Forbes is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and General Economics, Econometrics and Finance, having authored 21 papers that have together received 1.6k indexed citations. Recurring topics across this work include Solar and Space Plasma Dynamics (18 papers), Ionosphere and magnetosphere dynamics (13 papers), Astro and Planetary Science (9 papers), Geomagnetism and Paleomagnetism Studies (5 papers), Stellar, planetary, and galactic studies (3 papers), Magnetic confinement fusion research (2 papers), Solar Radiation and Photovoltaics (1 paper) and Gamma-ray bursts and supernovae (1 paper). The work is most often cited by research in Astronomy and Astrophysics (1.6k citations), Molecular Biology (420 citations) and Nuclear and High Energy Physics (77 citations). T. G. Forbes has collaborated with scholars based in United States, China and France. Frequent co-authors include Jun Lin, Philip A. Isenberg, Lin Jiao, P. Démoulin, E. R. Priest, A. Vourlidas, Jingjing Li, J. C. Raymond, Yuan‐Kuen Ko and Jun Lin. Their work appears in journals such as Science, Journal of Geophysical Research Atmospheres and The Astrophysical Journal.
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.