Ionospheric current system accompanied by auroral vortex streets
Yasutaka Hiraki

TL;DR
This paper investigates the formation of auroral vortex streets during substorms by analyzing ionospheric currents and Alfvén wave instabilities through magnetohydrodynamic simulations, revealing detailed current system behaviors.
Contribution
It provides a detailed physics-based explanation of ionospheric current systems associated with auroral vortex streets, emphasizing Cowling polarization effects and current balancing mechanisms.
Findings
Vortex street development involves balanced upward/downward pair currents.
Perturbed Hall and Pedersen currents are polarized eastward and point equatorward.
Current systems penetrate between pair currents, supporting vortex formation.
Abstract
High resolution optical measurements have revealed that a sudden brightening of aurora and its deformation from an arc-like to a vortex street structure appear just at the onset of substorm. The instability of Alfvn waves reflected from the ionosphere has been studied by means of magnetohydrodynamic simulations in order to comprehend the formation of auroral vortex streets. Our previous work reported that an initially placed arc intensifies, splits, and deforms into a vortex street during a couple of minutes, and the prime key is an enhancement of the convection electric field. This study elaborated physics of the ionospheric horizontal currents related to the vortex street in the context of so-called Cowling polarization. One component is due to the perturbed electric field by Alfvn waves, and the other is due to the perturbed electron density (or…
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Taxonomy
TopicsIonosphere and magnetosphere dynamics · Solar and Space Plasma Dynamics · Earthquake Detection and Analysis
