Preprints
https://doi.org/10.5194/egusphere-2026-11
https://doi.org/10.5194/egusphere-2026-11
30 Jan 2026
 | 30 Jan 2026
Status: this preprint is open for discussion and under review for Annales Geophysicae (ANGEO).

Flapping motion of onset aurora

Osuke Saka

Abstract. Onset aurora is meso-scale auroral forms (100s km) of spiral aurora arising out of the equatorward arc in association with the initial pulse of Pi2 pulsation, i.e., onset of field line dipolarization. Following the auroral onset, the head of the equatorward arc rapidly turns in a clockwise direction with expansion poleward, and during the second event of onset aurora, the whole of the arc rotates clockwise as viewed along the field lines. We model the deformation of onset aurora as an ExB drift of negatively charged solitary potential area (ion hole) in the polar ionosphere. It is suggested that twist motion of the onset aurora is analogous to the flapping motion of transmission belt in a factory driven by rotating line shaft. Like fluctuations in the line-of-sight velocity of the belt, non-uniform plasma flows in the ion hole trigger flapping motion of the arc.

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Osuke Saka

Status: open (until 13 Mar 2026)

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Osuke Saka
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Short summary
Pre-activated magnetosphere generates negatively charged solitary potential area in the polar ionosphere. Those areas act as auroral driver and form twist motion of auroral sheet. We suggest that twist motion of the auroral sheet is analogous to the flapping motion of transmission belt in a factory driven by rotating line shaft. Non-uniform shear flows in the auroral sheet trigger flapping instabilities.
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