MHD simulations of coronal dark downflows considering thermal conduction. Issue Volume 12:Issue S327(2016) (12th September 2017)

• Record Type: Journal Article
• Authors: Zurbriggen, E.; Costa, A.; Esquivel, A.; Schneiter, M.; Cécere, M.
• Editors: Vargas Domínguez, S.; Kosovichev, A.G.; Antolin, P.; Harra, L.
• Is Part Of: Proceedings of the International Astronomical Union. Volume 12:Issue S327(2016)
• Page Start: 128
• Page End: 133
• Publication Date: 2017-09-12
• Subjects: Sun: corona, -- magnetic fields, -- Physical Processes: MHD, -- conduction, -- instabilities, -- turbulence, -- shock waves; Astronomy -- Congresses; Astronomy -- Periodicals; 520
• DOI: 10.1017/S1743921317000217
• Languages: English
• ISSNs: 1743-9213

Abstract

Abstract: While several scenarios have been proposed to explain supra-arcade downflows (SADs) observed descending through turbulent hot regions, none of them have systematically addressed the consideration of thermal conduction. The SADs are known to be voided cavities. Our model assumes that SADs are triggered by bursty localized reconnection events that produce non-linear waves generating the voided cavity. These subdense cavities are sustained in time because they are hotter than their surrounding medium. Due to the low density and large temperature values of the plasma we expect the thermal conduction to be an important process. Our main aim here is to study if it is possible to generate SADs in the framework of our model considering thermal conduction. We carry on 2D MHD simulations including anisotropic thermal conduction, and find that if the magnetic lines envelope the cavities, they can be isolated from the hot environment and be identified as SADs.