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Multiwavelength Observations of a Slow Raise, Multi-Step X1.6 Flare and the Associated Eruption View all abstracts by submitter

Vasyl Yurchyshyn   Submitted: 2015-09-21 11:30

Using multi-wavelength observations we studied a slow rise, multi-step X1.6 flare that began on November 7, 2014 as a localized eruption of core fields inside a δ-sunspot and later engulfed the entire active region. This flare event was associated with formation of two systems of post eruption arcades and several J-shaped flare ribbons showing extremely fine details, irreversible changes in the photospheric magnetic fields, and it was accompanied by a fast and wide coronal mass ejection. Data from the Solar Dynamics Observatory, IRIS spacecraft along with the ground based data from the New Solar Telescope (NST) present evidence that i) the flare and the eruption were directly triggered by a flux emergence that occurred inside a δ-sunspot at the boundary between two umbrae; ii) this event represented an example of the formation of an unstable flux rope observed only in hot AIA channels (131 and 94 Å) and LASCO C2 coronagraph images; iii) the global post eruption arcade spanned the entire AR and was due to global scale reconnection occurring at heights of about one solar radii, indicating on the global spatial and temporal scale of the eruption.

Authors: Yurchyshyn, V., Kumar, P., Cho, K.S., Lim, E.K., & Abramenko, V.
Projects: IRIS,SDO-AIA,SDO-HMI

Publication Status: ApJ., accepted
Last Modified: 2015-09-23 13:32
Go to main E-Print page  Benchmark Test of Differential Emission Measure Codes and Multi-Thermal Energies in Solar Active Regions  Active region upflows: 2. Data driven MHD modeling  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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