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What is Nonaxisymmetric Instabilities in Solar Convection about?

Nonaxisymmetric instabilities can develop around magnetic flux tubes due to convection. The author uses numerical simulations of compressible magnetoconvection to investigate these instabilities. The simulations show both steady and oscillatory instabilities develop with preferred azimuthal wavenumbers. The unstable modes are located in the convecting region near the outer edge of the flux tube. Removing the magnetic field reveals these instabilities are driven by convection rather than magnetic effects. Hi

Author

Olmnop

Language

EN