Field Aligned Currents and Auroral Precipitation During the Terrestrial Alfven Wing State
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arXiv
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| Auteurs principaux: | , , , , , |
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| Format: | Preprint |
| Publié: |
2025
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| _version_ | 1866915276049612800 |
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| author | Burkholder, Brandon Chen, Li-Jen Sorathia, Kareem Lin, Dong Vines, Sarah Bowers, Charles F. |
| author_facet | Burkholder, Brandon Chen, Li-Jen Sorathia, Kareem Lin, Dong Vines, Sarah Bowers, Charles F. |
| contents | When sub-Alfvénic (Alfvén Mach number MA < 1) plasmas impact Earth, Alfvén wings (AWs) develop. A Multiscale Atmosphere Geospace Environment (MAGE) simulation of the April 2023 storm, validated by Active Magnetosphere and Planetary Electrodynamics Response Experiment (AMPERE) data, reveals the field-aligned-current (FAC) generation mechanism and predicts auroral precipitation for Earth's AWs. Simulation and observations show northern hemisphere planetward flowing electrons are predominantly at magnetic local times (MLTs) 8-13. Before the AWs formed, solar wind conditions were similar and MA ~ 1.4, yet the same FAC system extended from 9-18 MLT. Flow vorticity drives FACs at the boundary of the AWs and unshocked solar wind. The AW shape presents a different obstacle to the solar wind compared to typical lobe fluxes, producing the unique FAC distribution. New insights about AW FACs and precipitating electron energy flux will help understand auroral features for exoplanets inside their host star's Alfvén zone. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2502_16309 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Field Aligned Currents and Auroral Precipitation During the Terrestrial Alfven Wing State Burkholder, Brandon Chen, Li-Jen Sorathia, Kareem Lin, Dong Vines, Sarah Bowers, Charles F. Space Physics When sub-Alfvénic (Alfvén Mach number MA < 1) plasmas impact Earth, Alfvén wings (AWs) develop. A Multiscale Atmosphere Geospace Environment (MAGE) simulation of the April 2023 storm, validated by Active Magnetosphere and Planetary Electrodynamics Response Experiment (AMPERE) data, reveals the field-aligned-current (FAC) generation mechanism and predicts auroral precipitation for Earth's AWs. Simulation and observations show northern hemisphere planetward flowing electrons are predominantly at magnetic local times (MLTs) 8-13. Before the AWs formed, solar wind conditions were similar and MA ~ 1.4, yet the same FAC system extended from 9-18 MLT. Flow vorticity drives FACs at the boundary of the AWs and unshocked solar wind. The AW shape presents a different obstacle to the solar wind compared to typical lobe fluxes, producing the unique FAC distribution. New insights about AW FACs and precipitating electron energy flux will help understand auroral features for exoplanets inside their host star's Alfvén zone. |
| title | Field Aligned Currents and Auroral Precipitation During the Terrestrial Alfven Wing State |
| topic | Space Physics |
| url | https://arxiv.org/abs/2502.16309 |