Magnetic Twist and Writhe of Active Regions: On the Origin of Deformed Flux Tubes
M. L\'opez Fuentes, P. D\'emoulin, C.H. Mandrini, A.A. Pevtsov, L. van, Driel-Gesztelyi

TL;DR
This study investigates the deformation of magnetic flux tubes in active regions, examining the roles of kink-instability, Coriolis force, and large-scale flows in causing observed rotations and tilts.
Contribution
It provides a detailed analysis of the mechanisms behind flux tube deformation, including the first observational comparison of twist and writhe signs in active regions.
Findings
Kink-instability explains up to 35% of flux tube deformations.
Coriolis force accounts for about 36% of observed tilt changes.
Large-scale plasma flows may influence flux tube deformation beyond known mechanisms.
Abstract
We study the long term evolution of a set of 22 bipolar active regions (ARs) in which the main photospheric polarities are seen to rotate one around the other during several solar rotations. We first show that differential rotation is not at the origin of this large change in the tilt angle. A possible origin of this distortion is the nonlinear development of a kink-instability at the base of the convective zone; this would imply the formation of a non-planar flux tube which, while emerging across the photosphere, would show a rotation of its photospheric polarities as observed. A characteristic of the flux tubes deformed by this mechanism is that their magnetic twist and writhe should have the same sign. From the observed evolution of the tilt of the bipoles, we derive the sign of the writhe of the flux tube forming each AR; while we compute the sign of the twist from transverse field…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Astro and Planetary Science · Geomagnetism and Paleomagnetism Studies
