L. W. Acton
About
In The Last Decade
L. W. Acton
157 papers receiving 4.1k citations
Hit Papers
Peers
Comparison fields: 5 of 68
- Astronomy and Astrophysics 4.0k
- Molecular Biology 709
- Nuclear and High Energy Physics 358
- Atomic and Molecular Physics, and Optics 329
- Artificial Intelligence 238
Countries citing papers authored by L. W. Acton
This map shows the geographic impact of L. W. Acton'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 L. W. Acton with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites L. W. Acton more than expected).
Fields of papers citing papers by L. W. Acton
This network shows the impact of papers produced by L. W. Acton. 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 L. W. Acton. The network helps show where L. W. Acton may publish in the future.
Co-authorship network of co-authors of L. W. Acton
This figure shows the co-authorship network connecting the top 25 collaborators of L. W. Acton. A scholar is included among the top collaborators of L. W. Acton 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 L. W. Acton. L. W. Acton is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | The Point Spread Function of the Yohkoh Soft X-ray Telescope | 1 |
| 2 | Limb Events Observed by YOHKOH and Coronal Mass Ejections: A Filamentary Soft X-ray Structure on 5 October 1996 | 2 |
| 3 | Co-Temporal Evolution of Magnetic Sources of Coronal and Chromospheric/Photospheric Irradiance Variability | 1 |
| 4 | The TRACE Mission | 0 |
| 5 | The Solar-B Mission | 1 |
| 6 | 3 | |
| 7 | Microflaring at the Feet of Large Active Region Loops | 2 |
| 8 | The Dynamics of Coronal Holes as Determined From X-ray Synoptic Maps Derived From SXT Imagery | 3 |
| 9 | 25 | |
| 10 | Comparison between Hα and Yohkoh soft X-ray images of emerging flux regions | 2 |
| 11 | The soft X ray telescope for Solar-A | 0 |
| 12 | Performance of a solar soft X-ray spectrograph-telescope. | 1 |
| 13 | A Consistent Picture of Coronal and Chromospheric Processes in a Well-Observed Flare | 1 |
| 14 | Direct Evidence for Chromospheric Evaporation in a Well-Observed Compact Flare | 0 |
| 15 | Soft X-Ray Observations during the Preflare Phase of the Solar Flare Phenomenon. | 4 |
| 16 | The Early Evolution of X-Ray Producing Active Regions | 1 |
| 17 | Design and fabrication of multigrid X-ray collimators | 1 |
| 18 | Oxygen to Neon Abundance Ratio in the Solar Corona | 0 |
| 19 | Lockheed Solar Observatory, Saugus, California. Report 1967-1968. | 1 |
| 20 | X-Radiation of the Sun. | 2 |
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.