Field Aligned Currents and Aurora During the Terrestrial Alfven Wing State

When sub-Alfvenic (Alfven Mach number M_A < 1) plasmas impact Earth, the magnetosphere develops Alfven wings. A Multiscale Atmosphere Geospace Environment (MAGE) global simulation of the April 2023 geomagnetic storm, validated against Active Magnetosphere and Planetary Electrodynamics Response Experiment (AMPERE), reveals the mechanism of field-aligned current (FAC) generation and auroral precipitation for the terrestrial Alfven wings. Simulation and observations show northern hemisphere planetward flowing auroral electrons (negative FAC) are predominantly at magnetic local times (MLTs) 5-11. Just before the wings formed, solar wind conditions were similar and 1 < M_A < 2, yet negative FAC extended across the entire day-side and night-side dusk sectors. Flow vorticity drives FACs at the boundary of the Alfven wings and unshocked solar wind. The Alfven wing shape presents a different obstacle to the solar wind compared to typical lobe fluxes, producing the unique FAC and auroral patterns. New insights about Alfven wing FACs will generate new understanding of aurora for exoplanets inside their host star's Alfven zone.