Blob Formation and Ejection in Coronal Jets due to the Plasmoid and Kelvin–Helmholtz Instabilities
Ni,Lei1,2; Zhang,Qing-Min3; Murphy,Nicholas A.4; Lin,Jun1
Source PublicationThe Astrophysical Journal
AbstractAbstract We perform 2D resistive magnetohydrodynamic simulations of coronal jets driven by flux emergence along the lower boundary. The reconnection layers are susceptible to the formation of blobs that are ejected in the jet. Our simulation with low plasma β (Case I) shows that magnetic islands form easily and propagate upward in the jet. These islands are multithermal and thus are predicted to show up in hot channels (335 ? and 211 ?) and the cool channel (304 ?) in observations by the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory. The islands have maximum temperatures of 8 MK, lifetimes of 120 s, diameters of 6 Mm, and velocities of 200 km s?1. These parameters are similar to the properties of blobs observed in extreme-ultraviolet (EUV) jets by AIA. The Kelvin–Helmholtz instability develops in our simulation with moderately high plasma β (Case II) and leads to the formation of bright vortex-like blobs above the multiple high magnetosonic Mach number regions that appear along the jet. These vortex-like blobs can also be identified in the AIA channels. However, they eventually move downward and disappear after the high magnetosonic Mach number regions disappear. In the lower plasma β case, the lifetime for the jet is shorter, the jet and magnetic islands are formed with higher velocities and temperatures, the current-sheet fragments are more chaotic, and more magnetic islands are generated. Our results show that the plasmoid instability and Kelvin–Helmholtz instability along the jet are both possible causes of the formation of blobs observed at EUV wavelengths.
Keywordinstabilities magnetic reconnection magnetohydrodynamics (MHD) methods: numerical Sun: activity
WOS IDIOP:0004-637X-841-1-aa6ffe
PublisherThe American Astronomical Society
Citation statistics
Document Type期刊论文
Affiliation1.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, China;
2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, China
3.Key Laboratory for Dark Matter and Space Science, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China
4.Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
Recommended Citation
GB/T 7714
Ni,Lei,Zhang,Qing-Min,Murphy,Nicholas A.,等. Blob Formation and Ejection in Coronal Jets due to the Plasmoid and Kelvin–Helmholtz Instabilities[J]. The Astrophysical Journal,2017,841(1).
APA Ni,Lei,Zhang,Qing-Min,Murphy,Nicholas A.,&Lin,Jun.(2017).Blob Formation and Ejection in Coronal Jets due to the Plasmoid and Kelvin–Helmholtz Instabilities.The Astrophysical Journal,841(1).
MLA Ni,Lei,et al."Blob Formation and Ejection in Coronal Jets due to the Plasmoid and Kelvin–Helmholtz Instabilities".The Astrophysical Journal 841.1(2017).
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Ni,Lei]'s Articles
[Zhang,Qing-Min]'s Articles
[Murphy,Nicholas A.]'s Articles
Baidu academic
Similar articles in Baidu academic
[Ni,Lei]'s Articles
[Zhang,Qing-Min]'s Articles
[Murphy,Nicholas A.]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Ni,Lei]'s Articles
[Zhang,Qing-Min]'s Articles
[Murphy,Nicholas A.]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.