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Spectropolarimetric Insight into Plasma-Sheet Dynamics of a Solar Flare View all abstracts by submitter

Ryan French   Submitted: 2019-12-02 07:38

We examine spectropolarimetric data from the CoMP instrument, acquired during the evolution of the September 10th 2017 X8.2 solar flare on the western solar limb. CoMP captured linearly polarized light from two emission lines of Fe XIII at 1074.7 and 1079.8 nm, from 1.03 to 1.5 solar radii. We focus here on the hot plasma-sheet lying above the bright flare loops and beneath the ejected CME. The polarization has a striking and coherent spatial structure, with unexpectedly small polarization aligned with the plasma-sheet. By elimination, we find that small-scale magnetic field structure is needed to cause such significant depolarization, and suggest that plasmoid formation during reconnection (associated with the tearing mode instability) creates magnetic structure on scales below instrument resolution of 6 Mm. We conclude that polarization measurements with new coronagraphs, such as the upcoming DKIST, will further enhance our understanding of magnetic reconnection and development of turbulence in the solar corona.

Authors: Ryan J. French, Philip G. Judge, Sarah A. Matthews, Lidia van Driel-Gesztelyi
Projects: MLSO/CoMP,SDO-AIA

Publication Status: Accepted for publication to ApJ Letters
Last Modified: 2019-12-04 11:28
Go to main E-Print page  Magnetic Rayleigh-Taylor Instability at a Contact Discontinuity With   Oblique Magnetic Field  IRIS Mg II Observations and Non-LTE Modeling of Off-limb Spicules in a Solar Polar Coronal Hole  Edit Entry  Download Preprint  Delete Entry 

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