O. Aharonson
About
In The Last Decade
O. Aharonson
153 papers receiving 6.8k citations
Hit Papers
Peers
Comparison fields: 5 of 90
- Astronomy and Astrophysics 6.6k
- Atmospheric Science 2.3k
- Aerospace Engineering 1.2k
- Geophysics 548
- Molecular Biology 417
Countries citing papers authored by O. Aharonson
This map shows the geographic impact of O. Aharonson'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 O. Aharonson with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites O. Aharonson more than expected).
Fields of papers citing papers by O. Aharonson
This network shows the impact of papers produced by O. Aharonson. 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 O. Aharonson. The network helps show where O. Aharonson may publish in the future.
Co-authorship network of co-authors of O. Aharonson
This figure shows the co-authorship network connecting the top 25 collaborators of O. Aharonson. A scholar is included among the top collaborators of O. Aharonson 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 O. Aharonson. O. Aharonson 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 | The Science Mission of the SpaceIL Lunar Lander | 1 |
| 3 | 82 | |
| 4 | Shared origin for seven of Mars Trojans - impact ejecta from Mars? | 1 |
| 5 | A Multiple Impact Hypothesis for Moon Formation | 2 |
| 6 | Moon Formation from Multiple Large Impacts | 4 |
| 7 | Resolving the Great Drying of Mars: Paleo-Climate Versus Time from River Deposits in Aeolis Dorsa | 1 |
| 8 | Constraints on early Mars atmospheric pressure inferred from small ancient craters | 1 |
| 9 | 16 | |
| 10 | Roughness of lunar terrains: Slope statistics and power spectral density in cratering and diffusive equilibrium | 0 |
| 11 | Titan Mare Explorer (TiME): First In Situ Exploration of an Extraterrestrial Sea | 5 |
| 12 | Ontario Lacus: Brilliant Observations of a Titan Lake by the Cassini Radar Altimeter | 3 |
| 13 | Evidence for Liquid in Ontario Lacus (Titan) from Cassini-Observed Changes | 2 |
| 14 | Joint Analysis Of Titan's Surface Using The Cassini Vims And Radar Instruments. | 2 |
| 15 | The Nature and Origin of Mars' Intercrater Plains: New Insight from THEMIS | 2 |
| 16 | Stratigraphy and Structure of Inner Basin Outcrops in the Columbia Hills from the Spirit Rover | 1 |
| 17 | The Modern Impact Cratering Flux at the Surface of Mars | 3 |
| 18 | Why the Martian Mantle is (Mostly) "Wet" | 2 |
| 19 | Characterization of the Distributary Fan in Holden NE Crater Using Stereo Analysis | 5 |
| 20 | Geometry of Faults Underlying Wrinkle Ridges on Mars: Dynamic Modeling MOLA Topography | 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.