B. E. Goldstein
About
In The Last Decade
B. E. Goldstein
189 papers receiving 6.9k citations
Peers
Comparison fields: 5 of 102
- Astronomy and Astrophysics 7.6k
- Molecular Biology 2.2k
- Nuclear and High Energy Physics 451
- Atmospheric Science 407
- Geophysics 354
Countries citing papers authored by B. E. Goldstein
This map shows the geographic impact of B. E. Goldstein'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 B. E. Goldstein with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. E. Goldstein more than expected).
Fields of papers citing papers by B. E. Goldstein
This network shows the impact of papers produced by B. E. Goldstein. 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 B. E. Goldstein. The network helps show where B. E. Goldstein may publish in the future.
Co-authorship network of co-authors of B. E. Goldstein
This figure shows the co-authorship network connecting the top 25 collaborators of B. E. Goldstein. A scholar is included among the top collaborators of B. E. Goldstein 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 B. E. Goldstein. B. E. Goldstein is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 7 | |
| 2 | The evolution of the solar wind proton temperature anisotropy from 0.3 to 2.5 AU | 4 |
| 3 | 65 | |
| 4 | Velocity-space distribution functions of protons and alpha particles in the high-speed solar wind | 1 |
| 5 | The solar wind's return to a simple three-dimensional structure: Ulysses' second fast-latitude scan | 2 |
| 6 | 52 | |
| 7 | 113 | |
| 8 | 9 | |
| 9 | The Ulysses solar wind plasma investigation: Description and initial in-ecliptic results | 1 |
| 10 | Giotto IMS measurements of the production rate of hydrogen cyanide in the coma of comet Halley. | 14 |
| 11 | The pick-up of cometary protons by the solar wind | 38 |
| 12 | Measurements of the lunar induced magnetic moment in the geomagnetic tail - Evidence for a lunar core | 21 |
| 13 | Magnetic Evidence for a Lunar Core | 7 |
| 14 | Electrical conductivity of the lunar interior - Theory, error sources, and estimates | 4 |
| 15 | Lunar interaction with the solar wind - Effects on lunar electrical conductivity estimates | 4 |
| 16 | Energetic particles of the outer regions of planetary magnetospheres | 1 |
| 17 | The geomagnetic dynamos of the moon and Venus - Comparisons with a recent scaling law | 5 |
| 18 | Magnetic evidence concerning a lunar core | 13 |
| 19 | On the apparent diamagnetism of the lunar environment in the geomagnetic tail lobes | 7 |
| 20 | Lunar-Surface Solar-Wind Observations at the Apollo-12 and -15 Sites | 1 |
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.