Self-assembly of shallow magnetic spots through strongly stratified turbulence

Research output: Contribution to journalArticlepeer-review

40 Scopus citations


Recent studies have demonstrated that in fully developed turbulence, the effective magnetic pressure of a large-scale field (non-turbulent plus turbulent contributions) can become negative. In the presence of strongly stratified turbulence, this was shown to lead to a large-scale instability that produces spontaneous magnetic flux concentrations. Furthermore, using a horizontal magnetic field, elongated flux concentrations with a strength of a few percent of the equipartition value were found. Here we show that a uniform vertical magnetic field leads to circular magnetic spots of equipartition field strengths. This could represent a minimalistic model of sunspot formation and highlights the importance of two critical ingredients: turbulence and strong stratification. Radiation, ionization, and supergranulation may be important for realistic simulations, but are not critical at the level of a minimalistic model of magnetic spot formation.

Original languageEnglish
Article numberL23
JournalAstrophysical Journal Letters
Issue number2
StatePublished - 20 Oct 2013


  • magnetohydrodynamics (MHD)
  • starspots
  • sunspots
  • turbulence

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science


Dive into the research topics of 'Self-assembly of shallow magnetic spots through strongly stratified turbulence'. Together they form a unique fingerprint.

Cite this