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2.5D magnetohydrodynamic simulation of the formation and evolution of plasmoids in coronal current sheets
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dc.contributor.author | Mondal, Sripan | |
dc.contributor.author | Srivastava, Abhishek K. | |
dc.contributor.author | Pontin, David I. | |
dc.contributor.author | Yuan, Ding | |
dc.contributor.author | Priest, Eric R. | |
dc.date.accessioned | 2024-03-21T09:30:17Z | |
dc.date.available | 2024-03-21T09:30:17Z | |
dc.date.issued | 2024-03-07 | |
dc.identifier | 300189181 | |
dc.identifier | bdbc3e37-2153-45ba-9f32-facfe4373447 | |
dc.identifier | 85187401941 | |
dc.identifier.citation | Mondal , S , Srivastava , A K , Pontin , D I , Yuan , D & Priest , E R 2024 , ' 2.5D magnetohydrodynamic simulation of the formation and evolution of plasmoids in coronal current sheets ' , Astrophysical Journal , vol. 963 , no. 2 , 139 . https://doi.org/10.3847/1538-4357/ad2079 | en |
dc.identifier.issn | 0004-637X | |
dc.identifier.other | Bibtex: 2024ApJ...963..139M | |
dc.identifier.other | ORCID: /0000-0003-3621-6690/work/155626399 | |
dc.identifier.uri | https://hdl.handle.net/10023/29539 | |
dc.description | Funding: S.M. would like to acknowledge the financial support provided by the Prime Ministerʼs Research Fellowship of India. A.K.S. acknowledges the ISRO grant DS 2B-13012(2)/26/2022-Sec.2 for the support of his scientific research. D.I.P. gratefully acknowledges support through an Australian Research Council Discovery Project (DP210100709). D.Y. is supported by the National Natural Science Foundation of China (NSFC; grant Nos. 12173012, 12111530078, and 11803005), the Guangdong Natural Science Funds for Distinguished Young Scholar (grant No. 2023B1515020049), the Shenzhen Technology Project (grant No. GXWD20201230155427003-20200804151658001) and the Shenzhen Key Laboratory Launching Project (grant No. ZDSYS20210702140800001). | en |
dc.description.abstract | In the present paper, using MPI-AMRVAC, we perform a 2.5D numerical magnetohydrodynamic simulation of the dynamics and associated thermodynamical evolution of an initially force-free Harris current sheet subjected to an external velocity perturbation under the condition of uniform resistivity. The amplitude of the magnetic field is taken to be 10 G, typical of the solar corona. We impose a Gaussian velocity pulse across this current sheet that mimics the interaction of fast magnetoacoustic waves with a current sheet in the corona. This leads to a variety of dynamics and plasma processes in the current sheet, which is initially quasi-static. The initial pulse interacts with the current sheet and splits into a pair of counterpropagating wavefronts, which form a rarefied region that leads to an inflow and a thinning of the current sheet. The thinning results in Petschek-type magnetic reconnection followed by a tearing instability and plasmoid formation. The reconnection outflows containing outward-moving plasmoids have accelerated motions with velocities ranging from 105 to 303 km s−1. The average temperature and density of the plasmoids are found to be 8 MK and twice the background density of the solar corona, respectively. These estimates of the velocity, temperature, and density of the plasmoids are similar to values reported from various solar coronal observations. Therefore, we infer that the external triggering of a quasi-static current sheet by a single-velocity pulse is capable of initiating magnetic reconnection and plasmoid formation in the absence of a localized enhancement of resistivity in the solar corona. | |
dc.format.extent | 15 | |
dc.format.extent | 1369716 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astrophysical Journal | en |
dc.subject | Solar atmosphere | en |
dc.subject | Solar corona | en |
dc.subject | Magnetohydrodynamics | en |
dc.subject | Magnetic fields | en |
dc.subject | Solar magnetic reconnection | en |
dc.subject | QB Astronomy | en |
dc.subject | 3rd-NDAS | en |
dc.subject | NIS | en |
dc.subject | MCC | en |
dc.subject.lcc | QB | en |
dc.title | 2.5D magnetohydrodynamic simulation of the formation and evolution of plasmoids in coronal current sheets | en |
dc.type | Journal article | en |
dc.contributor.institution | University of St Andrews. Applied Mathematics | en |
dc.contributor.institution | University of St Andrews. School of Mathematics and Statistics | en |
dc.identifier.doi | https://doi.org/10.3847/1538-4357/ad2079 | |
dc.description.status | Peer reviewed | en |
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