Field-Aligned Currents and Auroral Precipitation During the Terrestrial Alfvén Wing State

B. L. Burkholder, L. J. Chen, D. Lin, S. K. Vines, K. A. Sorathia, C. F. Bowers

Research output: Contribution to journalArticlepeer-review

Abstract

When sub-Alfvénic (Alfvén Mach number (Formula presented.) 1) plasmas impact Earth, Alfvén wings (AWs) develop. A Multiscale Atmosphere Geospace Environment simulation of the April 2023 storm, validated by Active Magnetosphere and Planetary Electrodynamics Response Experiment 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 (Formula presented.), yet the same FAC system extended from 9 to 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.

Original languageEnglish
Article numbere2025GL115910
JournalGeophysical Research Letters
Volume52
Issue number12
DOIs
StatePublished - Jun 28 2025
Externally publishedYes

Keywords

  • Alfven wings
  • aurora
  • field-aligned current
  • geomagnetic storm
  • global magnetohydrodynamics
  • magnetic reconnection

Fingerprint

Dive into the research topics of 'Field-Aligned Currents and Auroral Precipitation During the Terrestrial Alfvén Wing State'. Together they form a unique fingerprint.

Cite this