G. E. Brueckner
About
In The Last Decade
G. E. Brueckner
42 papers receiving 450 citations
Peers
Comparison fields: 5 of 36
- Astronomy and Astrophysics 407
- Atomic and Molecular Physics, and Optics 97
- Atmospheric Science 85
- Molecular Biology 52
- Mechanics of Materials 49
Countries citing papers authored by G. E. Brueckner
This map shows the geographic impact of G. E. Brueckner'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 G. E. Brueckner with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. E. Brueckner more than expected).
Fields of papers citing papers by G. E. Brueckner
This network shows the impact of papers produced by G. E. Brueckner. 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 G. E. Brueckner. The network helps show where G. E. Brueckner may publish in the future.
Co-authorship network of co-authors of G. E. Brueckner
This figure shows the co-authorship network connecting the top 25 collaborators of G. E. Brueckner. A scholar is included among the top collaborators of G. E. Brueckner 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 G. E. Brueckner. G. E. Brueckner is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | A New View of the Solar Corona and the Solar Wind | 1 |
| 2 | Dynamical evolution of a coronal mass ejection (CME) to magnetic cloud: A preliminary analysis of the January 6-10, 1997 CME observed by LASCO/SOHO | 4 |
| 3 | Using LASCO Observations to Infer Solar Wind Flow Near the Sun | 3 |
| 4 | Description and Performance of the Recently Completed Naval Research Laboratory Solar Instrument Test Facility | 11 |
| 5 | Requirements for future solar-physics missions that include UV instrumentation. | 1 |
| 6 | The Large Angle Spectroscopic Coronagraph (LASCO): visible light coronal imaging and spectroscopy. | 1 |
| 7 | Correspondence between solar fine-scale structures in the corona, transition region, and lower atmosphere from collaborative observations | 1 |
| 8 | Results from the Solar Ultraviolet Spectral Irradiance Monitor Flown on Spacelab 2 | 0 |
| 9 | The Dynamics of Accelerating Coronal Bullets | 1 |
| 10 | HRTS Observations of Solar Fine Structure in the T min Region | 1 |
| 11 | Latitudinal Anisotropy of the Solar Far Ultraviolet Flux: Effect on the Lα Sky Background | 3 |
| 12 | Mass and Energy Flux in the Solar Transition Zone | 1 |
| 13 | An Analysis of High Spatial and Time Resolution C IV Line Profiles | 0 |
| 14 | High Spatial Resolution Cinematography of the 1600 Å Solar Continuum. | 1 |
| 15 | The UV Spectrum of a Sunspot (1175 to 1700 Å) Observed with High Spatial and Spectral Resolution | 1 |
| 16 | Interpreting XUV Spectroheliograms in Terms of Coronal Magnetic Field Structures | 2 |
| 17 | A New, High Resolution Ultraviolet Solar Spectrograph for Rocket and Satellite Applications. | 2 |
| 18 | The eruptive prominence of August 21, 1973 observed from Skylab in the white light corona and in the He II 304 Å chromosphere. | 2 |
| 19 | Absolute Intensity of the Solar Spectrum from 1200 Å to 1790 Å Derived from New Rocket Spectra | 1 |
| 20 | 4 |
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.