O. Hubickyj
About
In The Last Decade
O. Hubickyj
16 papers receiving 2.4k citations
Hit Papers
Peers
Comparison fields: 5 of 34
- Astronomy and Astrophysics 2.5k
- Instrumentation 259
- Spectroscopy 216
- Geophysics 110
- Atmospheric Science 72
Countries citing papers authored by O. Hubickyj
This map shows the geographic impact of O. Hubickyj'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. Hubickyj with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites O. Hubickyj more than expected).
Fields of papers citing papers by O. Hubickyj
This network shows the impact of papers produced by O. Hubickyj. 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. Hubickyj. The network helps show where O. Hubickyj may publish in the future.
Co-authorship network of co-authors of O. Hubickyj
This figure shows the co-authorship network connecting the top 25 collaborators of O. Hubickyj. A scholar is included among the top collaborators of O. Hubickyj 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. Hubickyj. O. Hubickyj is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | Models of Jupiter's Growth Incorporating Thermal and Hydrodynamics Constraints | 2 |
| 2 | 157 | |
| 3 | 247 | |
| 4 | 247 | |
| 5 | Evolution of Gas Giant Planets Using the Core Accretion Model | 2 |
| 6 | Direct Numerical Simulations of Turbulent Convection | 2 |
| 7 | Small Core for Jupiter using the Core Instability Model | 2 |
| 8 | Accumulation of Giant Planet Atmospheres Around Cores of a Few Earth Masses | 1 |
| 9 | New Models for the Formation of Jupiter | 1 |
| 10 | Formation of the Giant Planets by Concurrent Accretion of Solids and Gas breakdown → | 1765 |
| 11 | Simulations of the Accretion of the Giant Planets | 1 |
| 12 | 10 | |
| 13 | The role of turbulent convection in the primitive solar nebula. I - Theory. II - Results | 4 |
| 14 | 27 | |
| 15 | 48 | |
| 16 | 0 | |
| 17 | 16 |
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.