C. J. Crannell
- Astronomy and Astrophysics top 5%
- Solar and Space Plasma Dynamics 23
- Astrophysical Phenomena and Observations 9
- Gamma-ray bursts and supernovae 9
- Astro and Planetary Science 9
- Ionosphere and magnetosphere dynamics 8
- Nuclear and High Energy Physics top 10%
- Astrophysics and Cosmic Phenomena 9
- Particle Detector Development and Performance 8
- Radiation top 5%
- Nuclear Physics and Applications 9
- Partner nations
- United StatesSwitzerlandItaly
In The Last Decade
C. J. Crannell
55 papers receiving 628 citations
Peers
Comparison fields: 5 of 48
- Astronomy and Astrophysics 434
- Nuclear and High Energy Physics 221
- Radiation 131
- Geophysics 45
- Oceanography 24
Countries citing papers authored by C. J. Crannell
This map shows the geographic impact of C. J. Crannell'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. J. Crannell with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. J. Crannell more than expected).
Fields of papers citing papers by C. J. Crannell
This network shows the impact of papers produced by C. J. Crannell. 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. J. Crannell. The network helps show where C. J. Crannell may publish in the future.
Co-authorship network
The 25 scholars most cited alongside C. J. Crannell, 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 | The High Energy Solar Spectroscopic Imager - HESSI | 1996 | 3 |
| 2 | 1996 | 2 | |
| 3 | 1988 | 7 | |
| 4 | 1988 | 20 | |
| 5 | 1987 | 30 | |
| 6 | 1987 | 6 | |
| 7 | Cross sections for production of the 15.10 MeV and other astrophysically significant gamma-ray lines through excitation and spallation of 12 C and 16 O with protons | 1986 | 0 |
| 8 | 1985 | 94 | |
| 9 | Great microwave bursts and hard X rays from solar flares | 1983 | 1 |
| 10 | 1979 | 4 | |
| 11 | 1979 | 2 | |
| 12 | 1979 | 12 | |
| 13 | 1978 | 78 | |
| 14 | 1977 | 11 | |
| 15 | 1977 | 1 | |
| 16 | 1976 | 15 | |
| 17 | Positron Annihilation in Solar Flares | 1975 | 1 |
| 18 | 1974 | 5 | |
| 19 | CALIBRATION OF THE NASA--GSFC HIGH ENERGY COSMIC RAY EXPERIMENT. | 1971 | 1 |
| 20 | 1969 | 8 |
About C. J. Crannell
C. J. Crannell is a scholar working on Astronomy and Astrophysics, Radiation and Nuclear and High Energy Physics, having authored 57 papers that have together received 662 indexed citations. Recurring topics across this work include Solar and Space Plasma Dynamics (23 papers), Nuclear Physics and Applications (9 papers), Astrophysical Phenomena and Observations (9 papers), Gamma-ray bursts and supernovae (9 papers), Astrophysics and Cosmic Phenomena (9 papers), Astro and Planetary Science (9 papers), Ionosphere and magnetosphere dynamics (8 papers) and Particle Detector Development and Performance (8 papers). The work is most often cited by research in Astronomy and Astrophysics (434 citations), Nuclear and High Energy Physics (221 citations) and Radiation (131 citations). C. J. Crannell has collaborated with scholars based in United States, Switzerland and Italy. Frequent co-authors include R. Starr, R. J. Thomas, K. J. Frost, R. Ramaty, Carl Werntz, G. Joyce, K. Ohki, J. L. R. Saba, A. Magun and B. R. Dennis. Their work appears in journals such as Nature, Science 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.