Y. C. Saxena
- Nuclear and High Energy Physics top 5%
- Astronomy and Astrophysics top 5%
- Atomic and Molecular Physics, and Optics top 5%
- Electrical and Electronic Engineering
- Aerospace Engineering top 5%
- Topics
- Magnetic confinement fusion research (66 papers)Ionosphere and magnetosphere dynamics (39 papers)Superconducting Materials and Applications (34 papers)
- Cited by
- Nuclear and High Energy PhysicsAstronomy and AstrophysicsAtomic and Molecular Physics, and Optics
- Partner nations
- IndiaUnited StatesJapan
In The Last Decade
Y. C. Saxena
123 papers receiving 1.1k citations
Peers
Comparison fields: 5 of 77
- Nuclear and High Energy Physics 643
- Astronomy and Astrophysics 502
- Atomic and Molecular Physics, and Optics 384
- Electrical and Electronic Engineering 281
- Aerospace Engineering 210
Countries citing papers authored by Y. C. Saxena
This map shows the geographic impact of Y. C. Saxena'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 Y. C. Saxena with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Y. C. Saxena more than expected).
Fields of papers citing papers by Y. C. Saxena
This network shows the impact of papers produced by Y. C. Saxena. 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 Y. C. Saxena. The network helps show where Y. C. Saxena may publish in the future.
Co-authorship network of co-authors of Y. C. Saxena
This figure shows the co-authorship network connecting the top 25 collaborators of Y. C. Saxena. A scholar is included among the top collaborators of Y. C. Saxena 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 Y. C. Saxena. Y. C. Saxena is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 2 | |
| 2 | 2 | |
| 3 | 2 | |
| 4 | 0 | |
| 5 | 1 | |
| 6 | 2 | |
| 7 | 2 | |
| 8 | 6 | |
| 9 | 6 | |
| 10 | 7 | |
| 11 | 17 | |
| 12 | 7 | |
| 13 | 4 | |
| 14 | 1 | |
| 15 | 8 | |
| 16 | 3 | |
| 17 | 13 | |
| 18 | 18 | |
| 19 | 4 | |
| 20 | 1 |
About Y. C. Saxena
Y. C. Saxena is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Atomic and Molecular Physics, and Optics, having authored 128 papers that have together received 1.2k indexed citations. Recurring topics across this work include Magnetic confinement fusion research (66 papers), Ionosphere and magnetosphere dynamics (39 papers) and Superconducting Materials and Applications (34 papers). The work is most often cited by research in Nuclear and High Energy Physics (643 citations), Astronomy and Astrophysics (502 citations) and Atomic and Molecular Physics, and Optics (384 citations). Y. C. Saxena has collaborated with scholars based in India, United States and Japan. Frequent co-authors include P. I. John, R. Jha, S. K. Mattoo, P. K. Chattopadhyay, P. K. Kaw, C. V. S. Rao, Joydeep Ghosh, D. Bora, Arvindh Sekar and G. Prasad. Their work appears in journals such as Physical Review Letters, Journal of Applied Physics and Geophysical Research 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.