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  • Kemel, KoenKTH,Stockholms universitet,Nordiska institutet för teoretisk fysik (Nordita),Institutionen för astronomi,Nordic Institute for Theoretical Physics NORDITA (author)

Properties of the negative effective magnetic pressure instability

  • Article/chapterEnglish2012

Publisher, publication year, extent ...

  • 2012-02-13
  • Wiley,2012
  • printrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:su-80133
  • https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-80133URI
  • https://doi.org/10.1002/asna.201111638DOI
  • https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-95271URI

Supplementary language notes

  • Language:English
  • Summary in:English

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Classification

  • Subject category:ref swepub-contenttype
  • Subject category:art swepub-publicationtype

Notes

  • QC 20230922
  • As was demonstrated in earlier studies, turbulence can result in a negative contribution to the effective mean magnetic pressure, which, in turn, can cause a large-scale instability. In this study, hydromagnetic mean-field modelling is performed for an isothermally stratified layer in the presence of a horizontal magnetic field. The negative effective magnetic pressure instability (NEMPI) is comprehensively investigated. It is shown that, if the effect of turbulence on the mean magnetic tension force vanishes, which is consistent with results from direct numerical simulations of forced turbulence, the fastest growing eigenmodes of NEMPI are two-dimensional. The growth rate is found to depend on a parameter beta(star) characterizing the turbulent contribution of the effective mean magnetic pressure for moderately strong mean magnetic fields. A fit formula is proposed that gives the growth rate as a function of turbulent kinematic viscosity, turbulent magnetic diffusivity, the density scale height, and the parameter beta(star). The strength of the imposed magnetic field does not explicitly enter provided the location of the vertical boundaries are chosen such that the maximum of the eigenmode of NEMPI fits into the domain. The formation of sunspots and solar active regions is discussed as possible applications of NEMPI.

Subject headings and genre

Added entries (persons, corporate bodies, meetings, titles ...)

  • Brandenburg, AxelKTH,Stockholms universitet,Nordiska institutet för teoretisk fysik (Nordita),Institutionen för astronomi,Nordic Institute for Theoretical Physics NORDITA(Swepub:kth)u1os89mi (author)
  • Kleeorin, NathanKTH,Stockholms universitet,Nordiska institutet för teoretisk fysik (Nordita),Ben‐Gurion University of the Negev, Israel,Nordic Institute for Theoretical Physics NORDITA(Swepub:kth)u10pszpw (author)
  • Rogachevskii, IgorKTH,Stockholms universitet,Nordiska institutet för teoretisk fysik (Nordita),Ben‐Gurion University of the Negev, Israel,Nordic Institute for Theoretical Physics NORDITA(Swepub:kth)u1d6noho (author)
  • Stockholms universitetNordiska institutet för teoretisk fysik (Nordita) (creator_code:org_t)

Related titles

  • In:Astronomical Notes - Astronomische Nachrichten: Wiley333:2, s. 95-1000004-63371521-3994

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