Explosive events in active region observed by IRIS and SST/CRISP

Huang, Z., Madjarska, Maria, Scullion, Eamon, Xia, L.-D., Doyle, John Gerard and Ray, Tom (2017) Explosive events in active region observed by IRIS and SST/CRISP. Monthly Notices of the Royal Astronomical Society, 464 (2). pp. 1753-1761. ISSN 0035-8711

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Official URL: https://doi.org/10.1093/mnras/stw2469

Abstract

Transition-region explosive events (EEs) are characterized by non-Gaussian line profiles with enhanced wings at Doppler velocities of 50–150 km s−1. They are believed to be the signature of solar phenomena that are one of the main contributors to coronal heating. The aim of this study is to investigate the link of EEs to dynamic phenomena in the transition region and chromosphere in an active region. We analyse observations simultaneously taken by the Interface Region Imaging Spectrograph (IRIS) in the Si iv 1394 Å line and the slit-jaw (SJ) 1400 Å images, and the Swedish 1-m Solar Telescope in the Hα line. In total 24 events were found. They are associated with small-scale loop brightenings in SJ 1400 Å images. Only four events show a counterpart in the Hα−35 km s−1 and Hα+35 km s−1 images. Two of them represent brightenings in the conjunction region of several loops that are also related to a bright region (granular lane) in the Hα−35 km s−1 and Hα+35 km s−1 images. 16 are general loop brightenings that do not show any discernible response in the Hα images. Six EEs appear as propagating loop brightenings, from which two are associated with dark jet-like features clearly seen in the Hα−35 km s−1 images. We found that chromospheric events with jet-like appearance seen in the wings of the Hα line can trigger EEs in the transition region and in this case the IRIS Si iv 1394 Å line profiles are seeded with absorption components resulting from Fe ii and Ni ii. Our study indicates that EEs occurring in active regions have mostly upper-chromosphere/transition-region origin. We suggest that magnetic reconnection resulting from the braidings of small-scale transition region loops is one of the possible mechanisms of energy release that are responsible for the EEs reported in this paper.

Item Type: Article
Additional Information: This article has been accepted for publication in Monthly Notices of the Astronomical Society ©: 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Uncontrolled Keywords: methods: observational, techniques: spectroscopic, Sun: activity, Sun: chromosphere, Sun: transition region
Subjects: F500 Astronomy
Department: Faculties > Engineering and Environment > Mathematics and Information Sciences
Depositing User: Becky Skoyles
Date Deposited: 13 Mar 2017 16:54
Last Modified: 08 May 2017 19:18
URI: http://nrl.northumbria.ac.uk/id/eprint/30070

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