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dc.date.accessioned2024-04-30T15:23:31Z
dc.date.available2024-04-30T15:23:31Z
dc.date.created2024-04-17T14:16:41Z
dc.date.issued2024
dc.identifier.citationFærder, Øystein Håvard Nóbrega Siverio, Daniel Elias Carlsson, Mats . A comparative study of resistivity models for simulations of magnetic reconnection in the solar atmosphere. II. Plasmoid formation. Astronomy and Astrophysics (A & A). 2024, 683
dc.identifier.urihttp://hdl.handle.net/10852/110681
dc.description.abstractContext. Plasmoid-mediated reconnection plays a fundamental role in different solar atmospheric phenomena. Numerical reproduction of this process is therefore essential for developing robust solar models. Aims. Our goal is to assess plasmoid-mediated reconnection across various numerical resistivity models in order to investigate how plasmoid numbers and reconnection rates depend on the Lundquist number. Methods. We used the Bifrost code to drive magnetic reconnection in a 2D coronal fan-spine topology, carrying out a parametric study of several experiments with different numerical resolution and resistivity models. We employed three anomalous resistivity models: (1) the original hyper-diffusion from Bifrost, (2) a resistivity proportional to current density, and (3) a resistivity quadratically proportional to electron drift velocity. For comparisons, experiments with uniform resistivity were also run. Results. Plasmoid-mediated reconnection is obtained in most of the experiments. With uniform resistivity, increasing the resolution reveals higher plasmoid frequency with weaker scaling to the Lundquist number, obtaining 7.9–12 plasmoids per minute for S L  ∈ [1.8 × 10 4 , 2.6 × 10 5 ] with a scaling of S L 0.210 in the highest-resolution resistivity cases, transcending into Petschek reconnection in the high- S L limit (where the diffusive effects of the resistivity become small compared to the non-uniform viscosity) and Sweet-Parker reconnection in the low- S L limit. Anomalous resistivity leads to similar results even with lower resolution. The drift-velocity-dependent resistivity excellently reproduces Petschek reconnection for any Lundquist number, and similar results are seen with resistivity proportional to current-density though with slightly lower reconnection rates and plasmoid numbers. Among the different resistivity models applied on the given numerical resolution, the hyper-diffusion model reproduced plasmoid characteristics in closest resemblance to those obtained with uniform resistivity at a significantly higher resolution.
dc.languageEN
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleA comparative study of resistivity models for simulations of magnetic reconnection in the solar atmosphere. II. Plasmoid formation
dc.title.alternativeENEngelskEnglishA comparative study of resistivity models for simulations of magnetic reconnection in the solar atmosphere. II. Plasmoid formation
dc.typeJournal article
dc.creator.authorFærder, Øystein Håvard
dc.creator.authorNóbrega Siverio, Daniel Elias
dc.creator.authorCarlsson, Mats
cristin.unitcode185,15,3,40
cristin.unitnameRosseland senter for solfysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin2262399
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astronomy and Astrophysics (A & A)&rft.volume=683&rft.spage=&rft.date=2024
dc.identifier.jtitleAstronomy and Astrophysics (A & A)
dc.identifier.volume683
dc.identifier.pagecount13
dc.identifier.doihttps://doi.org/10.1051/0004-6361/202348046
dc.subject.nviVDP::Astrofysikk, astronomi: 438
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0004-6361
dc.type.versionPublishedVersion
cristin.articleidA95
dc.relation.projectNFR/262622


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