Y. A. Omelchenko
Physics and Astronomy · The Ohio State University
Publications
202
Citations
1,281
Est. group size
~1
Recurring co-author estimate
Active years
60
Publishing since 1967
Y. A. Omelchenko develops advanced computer simulations of space plasmas, focusing on how the solar wind interacts with Earth's magnetic environment (the magnetosphere and magnetosheath). This work uses hybrid simulation methods (which model ions individually while treating electrons as a fluid) and adaptive, multiscale computational techniques to study phenomena like magnetic reconnection, plasma shocks, ion outflow, and the structure of the magnetosheath and cusp regions. The research supports space weather modeling and is often shared as open-access simulation data, code, and visualization files.
Publication output has been fairly steady but variable over the last decade, with a slight recent decline in mean annual output (5.6/year over the last 5 years) compared to earlier peak years like 2019 and 2021.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- Advancing Heliophysics and Space Weather Modeling through Open Science
2026
- Recommendations for Advancing Heliophysics and Space Weather Modeling through Open Science
2026
- Advancing Heliophysics and Space Weather Modeling through Open Science
2026
- Data for "Adaptive Hybrid Modeling of Collisionless Plasma Shocks and Ion Acceleration"
Zenodo (CERN European Organization for Nuclear Research) · 2026
- Data for "Adaptive Hybrid Modeling of Collisionless Plasma Shocks and Ion Acceleration"
Zenodo (CERN European Organization for Nuclear Research) · 2026
- Movies for "Adaptive Hybrid Modeling of Collisionless Plasma Shocks and Ion Acceleration"
Zenodo (CERN European Organization for Nuclear Research) · 2026
- Movies for "Adaptive Hybrid Modeling of Collisionless Plasma Shocks and Ion Acceleration"
Zenodo (CERN European Organization for Nuclear Research) · 2026
- Simulation Models for Exploring Magnetic Reconnection
Space Science Reviews · 2025
- Flux Ropes Induced by O+ ${\mathrm{O}}^{+}$ Outflow in the Near‐Earth Magnetotail: Three‐Dimensional Hybrid Simulations
Geophysical Research Letters · 2024
- Simulation Models for Exploring Magnetic Reconnection
arXiv (Cornell University) · 2024
- Flux Ropes Induced by O+ Outflow in the Near-Earth Magnetotail: Three-Dimensional Hybrid Simulations
2024
- Soft X‐Ray Imaging of Earth's Dayside Magnetosheath and Cusps Using Hybrid Simulations
Geophysical Research Letters · 2023
- Multiscale hybrid modeling of the impact response of the Earth’s magnetotail to ionospheric O+ outflow
Frontiers in Astronomy and Space Sciences · 2023
- EMAPS: An Intelligent Agent-Based Technology for Simulation of Multiscale Systems
2023
- Commercial fishing of Pacific herring (Clupea pallasii) in January-April 2023 in the northern part of the Sea of Okhotsk
Fisheries · 2023
- Zenodo (CERN European Organization for Nuclear Research)×11
- AGU Fall Meeting Abstracts×8
- arXiv (Cornell University)×7
- Geophysical Research Letters×4
- Physics of Plasmas×3
- C. Carr
Physics and Astronomy · Purdue University West Lafayette
- Dong‐Hun Lee
Physics and Astronomy · Purdue University West Lafayette
- H. S. S. Sinha
Physics and Astronomy · Indiana University
- Y. Sahai
Physics and Astronomy · The Ohio State University
- Jin Wang
Physics and Astronomy · The Ohio State University
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 19, 2026.
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