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Dynamics of Late-Stage Reconnection in the 2017 September 10 Solar Flare View all abstracts by submitter

Ryan French   Submitted: 2020-07-28 09:50

In this multi-instrument paper, we search for evidence of sustained magnetic reconnection far beyond the impulsive phase of the X8.2-class solar flare on 2017 September 10. Using Hinode/EIS, CoMP, SDO/AIA, K-Cor, Hinode/XRT, RHESSI, and IRIS, we study the late-stage evolution of the flare dynamics and topology, comparing signatures of reconnection with those expected from the standard solar flare model. Examining previously unpublished EIS data, we present the evolution of non-thermal velocity and temperature within the famous plasma sheet structure, for the first four hours of the flare's duration. On even longer time scales, we use Differential Emission Measures and polarization data to study the longevity of the flare's plasma sheet and cusp structure, discovering that the plasma sheet is still visible in CoMP linear polarization observations on 2017 September 11, long after its last appearance in EUV. We deduce that magnetic reconnection of some form is still ongoing at this time - 27 hours after flare onset.

Authors: Ryan J. French, Sarah A. Matthews, Lidia van Driel-Gesztelyi, David M. Long, Philip G. Judge
Projects: MLSO/CoMP,Hinode/EIS,Hinode/XRT,IRIS,RHESSI,SDO-AIA

Publication Status: Accepted for publication to ApJ
Last Modified: 2020-07-29 13:06
Go to main E-Print page  Solar Flare Arcade Modelling: Bridging the gap from 1D to 3D Simulations of Optically Thin Radiation  Polarisation and source structure of solar stationary type IV radio bursts  Edit Entry  Download Preprint  Delete Entry 

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