C. E. Parnell
- Astronomy and Astrophysics top 1%
- Solar and Space Plasma Dynamics 76
- Ionosphere and magnetosphere dynamics 49
- Astro and Planetary Science 28
- Stellar, planetary, and galactic studies 21
- Lightning and Electromagnetic Phenomena 1
- Nuclear and High Energy Physics top 10%
- Magnetic confinement fusion research 11
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- Geomagnetism and Paleomagnetism Studies 30
- Artificial Intelligence top 10%
- Solar Radiation and Photovoltaics 3
C. E. Parnell
78 papers receiving 2.3k citations
Peers
Comparison fields: 5 of 44
- Astronomy and Astrophysics 2.3k
- Nuclear and High Energy Physics 220
- Molecular Biology 670
- Artificial Intelligence 159
- Geophysics 42
Countries citing papers authored by C. E. Parnell
This map shows the geographic impact of C. E. Parnell'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 C. E. Parnell with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. E. Parnell more than expected).
Fields of papers citing papers by C. E. Parnell
This network shows the impact of papers produced by C. E. Parnell. 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 C. E. Parnell. The network helps show where C. E. Parnell may publish in the future.
Co-authorship network
The 25 scholars most cited alongside C. E. Parnell, 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 | 2025 | 1 | |
| 2 | 2020 | 5 | |
| 3 | 2020 | 6 | |
| 4 | 2019 | 18 | |
| 5 | 2019 | 9 | |
| 6 | 2016 | 12 | |
| 7 | 2015 | 35 | |
| 8 | 2015 | 12 | |
| 9 | 2014 | 9 | |
| 10 | 2014 | 31 | |
| 11 | 2010 | 11 | |
| 12 | 2009 | 14 | |
| 13 | 2008 | 33 | |
| 14 | The Small-Scale Field Measured With Hinode/SOT and Feature Tracking: Where is the mixed- polarity flux? | 2008 | 0 |
| 15 | Feature Tracking of Hinode Magnetograms | 2007 | 0 |
| 16 | 3D magnetic reconnection, flares and coronal heating | 2007 | 1 |
| 17 | 2005 | 15 | |
| 18 | 2005 | 28 | |
| 19 | 2005 | 8 | |
| 20 | Comparison of Blinkers and Explosive Events | 2003 | 1 |
About C. E. Parnell
C. E. Parnell is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Molecular Biology, having authored 82 papers that have together received 2.4k indexed citations. Recurring topics across this work include Solar and Space Plasma Dynamics (76 papers), Ionosphere and magnetosphere dynamics (49 papers), Geomagnetism and Paleomagnetism Studies (30 papers), Astro and Planetary Science (28 papers), Stellar, planetary, and galactic studies (21 papers), Magnetic confinement fusion research (11 papers), Solar Radiation and Photovoltaics (3 papers) and Lightning and Electromagnetic Phenomena (1 paper). The work is most often cited by research in Astronomy and Astrophysics (2.3k citations), Nuclear and High Energy Physics (220 citations) and Molecular Biology (670 citations). C. E. Parnell has collaborated with scholars based in United Kingdom, United States and Germany. Frequent co-authors include E. R. Priest, A. L. Haynes, P. E. Jupp, K. Galsgaard, I. De Moortel, T. Neukirch, Markus J. Aschwanden, S. F. Martin, J. M. Smith and L. Golub. Their work appears in journals such as Astronomy and Astrophysics, Solar Physics, The Astrophysical Journal, Physics of Plasmas and Geophysical & Astrophysical Fluid Dynamics.
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.