E. T. Sarris
About
In The Last Decade
E. T. Sarris
174 papers receiving 2.4k citations
Peers
Comparison fields: 5 of 63
- Astronomy and Astrophysics 2.6k
- Geophysics 657
- Molecular Biology 643
- Nuclear and High Energy Physics 493
- Electrical and Electronic Engineering 155
Countries citing papers authored by E. T. Sarris
This map shows the geographic impact of E. T. Sarris'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 E. T. Sarris with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. T. Sarris more than expected).
Fields of papers citing papers by E. T. Sarris
This network shows the impact of papers produced by E. T. Sarris. 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 E. T. Sarris. The network helps show where E. T. Sarris may publish in the future.
Co-authorship network of co-authors of E. T. Sarris
This figure shows the co-authorship network connecting the top 25 collaborators of E. T. Sarris. A scholar is included among the top collaborators of E. T. Sarris 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 E. T. Sarris. E. T. Sarris is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 16 | |
| 2 | Occurrence of high-beta superthermal plasma conditions in the interplanetary medium | 3 |
| 3 | Spatial Distribution, Composition and Charge State of Energetic Ions Upstream from the Kronian Magnetosphere | 3 |
| 4 | A CMOS time to digital converter for space science instruments | 4 |
| 5 | A 10 bit, low power, digitally auto–zeroed CMOS analogue to digital converter core for the NASA TRIO smart sensor system on a chip | 6 |
| 6 | Energetic proton fluxes within the magnetosheath and upstream from the bow shock: Interball-1 data | 4 |
| 7 | 0 | |
| 8 | The DOK-2 Experiment to Study Energetic Particles by the Tail Probe and Auroral Probe Satellites in the INTERBALL Project | 32 |
| 9 | Bidirectional Particle Fluxes in Magnetic Clouds and their Environs | 1 |
| 10 | Solar Flare Electrons Propagation in Converging Interplanetary Magnetic Structures | 2 |
| 11 | AMPTE/CCE CHEM observations of the energetic ion population at geosynchronous altitudes | 78 |
| 12 | A preliminary low-dimensional chaotic analysis of the solar cycle | 5 |
| 13 | Long-period standing waves at the Plasma Sheet Boundary Layer region observed by ISEE-1 | 6 |
| 14 | Low Energy Ion and Electron Measurements of the March-April 1991 Solar Events by Ulysses | 1 |
| 15 | Encounter with a source of energetic particles inside the plasma sheet | 3 |
| 16 | Entry of solar energetic protons into the distant plasma sheet - dependence on distance from the neutral sheet | 1 |
| 17 | Characteristics of particle events associated with interplanetary shocks. | 1 |
| 18 | ISEE-3 observations of interplanetary shock accelerated protons | 8 |
| 19 | Observations of quiet-time interplanetary electron enhancements of Jovian origin | 5 |
| 20 | Effects of Interplanetary Shock Waves on Energetic Charged-Particles | 98 |
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.