Ka Ho Yuen
- Astronomy and Astrophysics top 5%
- Atmospheric Science
- Atomic and Molecular Physics, and Optics
- Spectroscopy
- Nuclear and High Energy Physics
- Co-authors
- A. LazarianYue HuHuirong YanD. PogosyanHyeseung LeePo Kin LeungQizhou ZhangT. K. Sridharan
- Topics
- Astrophysics and Star Formation Studies (21 papers)Solar and Space Plasma Dynamics (19 papers)Stellar, planetary, and galactic studies (14 papers)
- Partner nations
- United StatesGermanyChile
In The Last Decade
Ka Ho Yuen
27 papers receiving 418 citations
Peers
Comparison fields: 5 of 25
- Astronomy and Astrophysics 460
- Atmospheric Science 44
- Atomic and Molecular Physics, and Optics 38
- Spectroscopy 30
- Nuclear and High Energy Physics 26
Countries citing papers authored by Ka Ho Yuen
This map shows the geographic impact of Ka Ho Yuen'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 Ka Ho Yuen with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Ka Ho Yuen more than expected).
Fields of papers citing papers by Ka Ho Yuen
This network shows the impact of papers produced by Ka Ho Yuen. 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 Ka Ho Yuen. The network helps show where Ka Ho Yuen may publish in the future.
Co-authorship network of co-authors of Ka Ho Yuen
This figure shows the co-authorship network connecting the top 25 collaborators of Ka Ho Yuen. A scholar is included among the top collaborators of Ka Ho Yuen 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 Ka Ho Yuen. Ka Ho Yuen is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 11 | |
| 3 | 2 | |
| 4 | 2 | |
| 5 | 5 | |
| 6 | 4 | |
| 7 | 4 | |
| 8 | 10 | |
| 9 | 6 | |
| 10 | 10 | |
| 11 | 10 | |
| 12 | 4 | |
| 13 | 14 | |
| 14 | 15 | |
| 15 | Improving Velocity Gradient Technique with Principal Component Analysis | 1 |
| 16 | Diagnostics of turbulence properties through Velocity Gradient Amplitudes: Theory and Observations | 4 |
| 17 | 35 | |
| 18 | 60 | |
| 19 | 76 | |
| 20 | 9 |
About Ka Ho Yuen
Ka Ho Yuen is a scholar working on Astronomy and Astrophysics, Oceanography and Fluid Flow and Transfer Processes, having authored 27 papers that have together received 481 indexed citations. Recurring topics across this work include Astrophysics and Star Formation Studies (21 papers), Solar and Space Plasma Dynamics (19 papers) and Stellar, planetary, and galactic studies (14 papers). The work is most often cited by research in Astronomy and Astrophysics (460 citations), Atmospheric Science (44 citations) and Nuclear and High Energy Physics (26 citations). Ka Ho Yuen has collaborated with scholars based in United States, Germany and Chile. Frequent co-authors include A. Lazarian, Yue Hu, Huirong Yan, D. Pogosyan, Hyeseung Lee, Po Kin Leung, Qizhou Zhang, T. K. Sridharan, Ya‐Wen Tang and Hauyu Baobab Liu. Their work appears in journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.
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.