Hide metadata

dc.date.accessioned2022-10-07T17:11:36Z
dc.date.available2022-10-07T17:11:36Z
dc.date.created2022-09-16T10:34:42Z
dc.date.issued2022
dc.identifier.citationMoreno-Insertis, F. Nóbrega Siverio, Daniel Elias Priest, E.R. Hood, A.W. . Ambipolar diffusion: Self-similar solutions and MHD code testing: Cylindrical symmetry. Astronomy and Astrophysics (A & A). 2022, 662
dc.identifier.urihttp://hdl.handle.net/10852/97082
dc.description.abstractContext. Ambipolar diffusion is a process occurring in partially ionised astrophysical systems that imparts a complicated mathematical and physical nature to Ohm’s law. The numerical codes that solve the magnetohydrodynamic (MHD) equations have to be able to deal with the singularities that are naturally created in the system by the ambipolar diffusion term. Aims. The global aim is to calculate a set of theoretical self-similar solutions to the nonlinear diffusion equation with cylindrical symmetry that can be used as tests for MHD codes which include the ambipolar diffusion term. Methods. First, following the general methods developed in the applied mathematics literature, we obtained the theoretical solutions as eigenfunctions of a nonlinear ordinary differential equation. Phase-plane techniques were used to integrate through the singularities at the locations of the nulls, which correspond to infinitely sharp current sheets. In the second half of the paper, we consider the use of these solutions as tests for MHD codes. To that end, we used the Bifrost code, thereby testing the capabilities of these solutions as tests as well as (inversely) the accuracy of Bifrost’s recently developed ambipolar diffusion module. Results. The obtained solutions are shown to constitute a demanding, but nonetheless viable, test for MHD codes that incorporate ambipolar diffusion. Detailed tabulated runs of the solutions have been made available at a public repository. The Bifrost code is able to reproduce the theoretical solutions with sufficient accuracy up to very advanced diffusive times. Using the code, we also explored the asymptotic properties of our theoretical solutions in time when initially perturbed with either small or finite perturbations. Conclusions. The functions obtained in this paper are relevant as physical solutions and also as tests for general MHD codes. They provide a more stringent and general test than the simple Zeldovich-Kompaneets-Barenblatt-Pattle solution.
dc.languageEN
dc.titleAmbipolar diffusion: Self-similar solutions and MHD code testing: Cylindrical symmetry
dc.title.alternativeENEngelskEnglishAmbipolar diffusion: Self-similar solutions and MHD code testing: Cylindrical symmetry
dc.typeJournal article
dc.creator.authorMoreno-Insertis, F.
dc.creator.authorNóbrega Siverio, Daniel Elias
dc.creator.authorPriest, E.R.
dc.creator.authorHood, A.W.
cristin.unitcode185,15,3,40
cristin.unitnameRosseland senter for solfysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin2052372
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=662&rft.spage=&rft.date=2022
dc.identifier.jtitleAstronomy and Astrophysics (A & A)
dc.identifier.volume662
dc.identifier.pagecount14
dc.identifier.doihttps://doi.org/10.1051/0004-6361/202141449
dc.subject.nviVDP::Astrofysikk, astronomi: 438
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0004-6361
dc.type.versionPublishedVersion
cristin.articleidA42
dc.relation.projectNFR/262622


Files in this item

Appears in the following Collection

Hide metadata