Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7176
Title: Successive Homologous Coronal Mass Ejections Driven by Shearing and Converging Motions in Solar Active Region NOAA 12371
Authors: Vemareddy, P
Keywords: Sun: activity;Sun: coronal mass ejections (CMEs);Sun: evolution;Sun: filaments, prominences;Sun: heliosphere;Sun: magnetic fields
Issue Date: 20-Aug-2017
Publisher: IOP Publishing
Citation: The Astrophysical Journal, Vol. 845, No. 1, 59
Abstract: We study the magnetic field evolution in AR 12371, related to its successive eruptive nature. During the disk transit of seven days, the active region (AR) launched four sequential fast coronal mass ejections (CMEs), which are associated with long duration M-class flares. Morphological study delineates a pre-eruptive coronal sigmoid structure above the polarity inversion line (PIL) similar to Moore et al.'s study. The velocity field derived from tracked magnetograms indicates persistent shear and converging motions of polarity regions about the PIL. While these shear motions continue, the crossed arms of two sigmoid elbows are being brought to interaction by converging motions at the middle of the PIL, initiating the tether-cutting reconnection of field lines and the onset of the CME explosion. The successive CMEs are explained by a cyclic process of magnetic energy storage and release referred to as "sigmoid-to-arcade-to-sigmoid" transformation driven by photospheric flux motions. Furthermore, the continued shear motions inject helicity flux with a dominant negative sign, which contributes to core field twist and its energy by building a twisted flux rope (FR). After a limiting value, the excess coronal helicity is expelled by bodily ejection of the FR, which is initiated by some instability as realized by intermittent CMEs. This AR is in contrast with the confined AR 12192 with a predominant negative sign and larger helicity flux, but much weaker (−0.02 turns) normalized coronal helicity content. While predominant signed helicity flux is a requirement for CME eruption, our study suggests that the magnetic flux normalized helicity flux is a necessary condition accommodating the role of background flux and appeals to a further study of a large sample of ARs.
Description: Restricted Access
URI: http://hdl.handle.net/2248/7176
ISSN: 0004-637X
???metadata.dc.rights???: © The American Astronomical Society
???metadata.dc.relation.uri???: https://doi.org/10.3847/1538-4357/aa7ff4
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Successive_Homologous_Coronal_Mass_Ejections_Driven.pdfRestricted Access6.76 MBAdobe PDFView/Open    Request a copy


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.