Transient Coronal Sigmoids and Rotating Erupting Flux Ropes

Details Transient Coronal Sigmoids and Rotating Erupting Flux Ropes Transient Coronal Sigmoids and Rotating Erupting Flux Ropes

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007soph..246..365g&link_type=abstract

Solar Physics, Volume 246, Issue 2, pp.365-391

Physics

60

Sun: Sigmoids, Sun: Flux Rope, Sun: Magnetic Fields, Sun: Eruptions

Scientific paper

To determine the relationship between transient coronal (soft X-ray or EUV) sigmoids and erupting flux ropes, we analyse four events in which a transient sigmoid could be associated with a filament whose apex rotates upon eruption and two further events in which the two phenomena were spatially but not temporally coincident. We find the helicity sign of the erupting field and the direction of filament rotation to be consistent with the conversion of twist into writhe under the ideal MHD constraint of helicity conservation, thus supporting our assumption of flux rope topology for the rising filament. For positive (negative) helicity the filament apex rotates clockwise (counterclockwise), consistent with the flux rope taking on a reverse (forward) S shape, which is opposite to that observed for the sigmoid. This result is incompatible with two models for sigmoid formation: one identifying sigmoids with upward arching kink-unstable flux ropes and one identifying sigmoids with a current layer between two oppositely sheared arcades. We find instead that the observations agree well with the model by Titov and Démoulin ( Astron. Astrophys. 351, 707, 1999), which identifies transient sigmoids with steepened current layers below rising flux ropes.

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