A. B. Galvin
About
In The Last Decade
A. B. Galvin
159 papers receiving 4.7k citations
Peers
Comparison fields: 5 of 81
- Astronomy and Astrophysics 4.7k
- Molecular Biology 1.3k
- Geophysics 395
- Atmospheric Science 356
- Nuclear and High Energy Physics 255
Countries citing papers authored by A. B. Galvin
This map shows the geographic impact of A. B. Galvin'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 A. B. Galvin with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. B. Galvin more than expected).
Fields of papers citing papers by A. B. Galvin
This network shows the impact of papers produced by A. B. Galvin. 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 A. B. Galvin. The network helps show where A. B. Galvin may publish in the future.
Co-authorship network of co-authors of A. B. Galvin
This figure shows the co-authorship network connecting the top 25 collaborators of A. B. Galvin. A scholar is included among the top collaborators of A. B. Galvin 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 A. B. Galvin. A. B. Galvin 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 | 8 | |
| 3 | 8 | |
| 4 | 24 | |
| 5 | 11 | |
| 6 | 30 | |
| 7 | 9 | |
| 8 | Direction and orientation of CME/ICME events observed by STEREO | 1 |
| 9 | CMEs In The Heliosphere Observed With Combined Imaging And In-situ Data From LASCO, Stereo And SMEI | 1 |
| 10 | Manifestations of solar differential rotation in the solar wind: An update | 1 |
| 11 | Do in Situ Observations of Solar Wind Stream Interfaces Reflect the Evolution of Coronal Holes | 1 |
| 12 | Flare and Erupting Filament of 19th May, 2007 - Sources of a Magnetic Cloud Observed by Stereo | 1 |
| 13 | Charge states of energetic (approximate to 0.5 MeV/n) ions in corotating interaction regions at 1 AU and implications on source populations | 7 |
| 14 | Measurement of the Ar/Ca Abundance Ratio From CELIAS/MTOF in Slow and Fast Solar Wind | 1 |
| 15 | Variation of Energetic He + , He 2+ and Heavy Ions Across Co-Rotating Interaction Regions | 1 |
| 16 | 24 | |
| 17 | The iron, silicon, and oxygen abundance in the solar wind measured with SOHO/CELIAS/MTOF | 3 |
| 18 | Coronal Abundances: What are They? | 3 |
| 19 | Proton Temperatures, Electron Temperatures and Outflows in the Extended Solar Corona. | 2 |
| 20 | Energetic (greater than 100 keV) O(+) ions in the plasma sheet | 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.