UCL Discovery Stage
UCL home » Library Services » Electronic resources » UCL Discovery Stage

The Merging of a Coronal Dimming and the Southern Polar Coronal Hole

Ngampoopun, Nawin; Long, David M; Baker, Deborah; Green, Lucie M; Yardley, Stephanie L; James, Alexander W; To, Andy SH; (2023) The Merging of a Coronal Dimming and the Southern Polar Coronal Hole. The Astrophysical Journal , 950 (2) , Article 150. 10.3847/1538-4357/acd44e. Green open access

[thumbnail of Ngampoopun_2023_ApJ_950_150.pdf]
Preview
Text
Ngampoopun_2023_ApJ_950_150.pdf - Published Version

Download (1MB) | Preview

Abstract

We report on the merging between the southern polar coronal hole and an adjacent coronal dimming induced by a coronal mass ejection on 2022 March 18, resulting in the merged region persisting for at least 72 hr. We use remote sensing data from multiple co-observing spacecraft to understand the physical processes during this merging event. The evolution of the merger is examined using Extreme-UltraViolet (EUV) images obtained from the Atmospheric Imaging Assembly on board the Solar Dynamic Observatory and Extreme Ultraviolet Imager, which is on board the Solar Orbiter spacecraft. The plasma dynamics are quantified using spectroscopic data obtained from the EUV Imaging Spectrometer on board Hinode. The photospheric magnetograms from the Helioseismic and Magnetic Imager are used to derive the magnetic field properties. To our knowledge, this work is the first spectroscopical analysis of the merging of two open-field structures. We find that the coronal hole and the coronal dimming become indistinguishable after the merging. The upflow speeds inside the coronal dimming become more similar to that of a coronal hole, with a mixture of plasma upflows and downflows observable after the merging. The brightening of the bright points and the appearance of coronal jets inside the merged region further imply ongoing reconnection processes. We propose that component reconnection between the coronal hole and coronal dimming fields plays an important role during this merging event because the footpoint switching resulting from the reconnection allows the coronal dimming to intrude onto the boundary of the southern polar coronal hole.

Type: Article
Title: The Merging of a Coronal Dimming and the Southern Polar Coronal Hole
Open access status: An open access version is available from UCL Discovery
DOI: 10.3847/1538-4357/acd44e
Publisher version: https://doi.org/10.3847/1538-4357/acd44e
Language: English
Additional information: Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10172548
Downloads since deposit
684Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item