Is flare-ribbon fine structure related to tearing in the flare current sheet?
P. F. Wyper, D. I. Pontin

TL;DR
This study links fine structures in solar flare ribbons, such as spirals and waves, to tearing instabilities in the flare current sheet, supported by an analytical magnetic field model and analysis of the squashing factor.
Contribution
It introduces a 3D magnetic field model showing how tearing modes can produce observed flare ribbon fine structures, establishing a direct connection.
Findings
Flare ribbon fine structures are related to oblique tearing modes.
Spiral and wave features depend on flux rope size, location, and twist.
Handedness of spirals matches that of the main ribbon hooks.
Abstract
Observations of solar flare ribbons show significant fine structure in the form of breaking wave-like perturbations and spirals. The origin of this structure is not well understood, but one possibility is that it is related to the tearing instability in the flare current sheet. Here we study this connection by constructing an analytical three-dimensional magnetic field representative of an erupting flux rope with a flare current sheet below it. We introduce small-scale flux ropes representative of those formed during a tearing instability in the current layer, and use the squashing factor on the solar surface to identify the shape of the presumed flare ribbons and fine structure. Our analysis suggests there is a direct link between flare-ribbon fine structure and flare current sheet tearing, with the majority of the ribbon fine structure related to oblique tearing modes. Depending upon…
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