Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6838
Title: Investigation of helicity and energy flux transport in three emerging solar active regions
Authors: Vemareddy, P
Keywords: Sun: corona;Sun: coronal mass ejections (CMEs);Sun: evolution;Sun: flares;Sun: magnetic fields;Sun: photosphere
Issue Date: 20-Jun-2015
Publisher: IOP Publishing
Citation: The Astrophysical Journal, Vol. 806, No. 2, 245
Abstract: We report the results of an investigation of helicity and energy flux transport from three emerging solar active regions (ARs). Using time sequence vector magnetic field observations obtained from the Helioseismic Magnetic Imager, the velocity field of plasma flows is derived by the differential affine velocity estimator for vector magnetograms. In three cases, the magnetic fluxes evolve to pump net positive, negative, and mixed-sign helicity flux into the corona. The coronal helicity flux is dominantly coming from the shear term that is related to horizontal flux motions, whereas energy flux is dominantly contributed by the emergence term. The shear helicity flux has a phase delay of 5–14 hr with respect to absolute magnetic flux. The nonlinear curve of coronal energy versus relative helicity identifies the configuration of coronal magnetic fields, which is approximated by a fit of linear force-free fields. The nature of coronal helicity related to the particular pattern of evolving magnetic fluxes at the photosphere has implications for the generation mechanism of two kinds of observed activity in the ARs.
Description: Restricted Access
URI: http://hdl.handle.net/2248/6838
ISSN: 0004-637X
???metadata.dc.rights???: © The American Astronomical Society
???metadata.dc.relation.uri???: http://dx.doi.org/10.1088/0004-637X/806/2/245
Appears in Collections:IIAP Publications

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