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Nonlinear slow magnetoacoustic waves in coronal plasma structures View all abstracts by submitter

Valery Nakariakov   Submitted: 2014-11-02 06:27

Context. There is abundant observational evidence of longitudinal waves in the plasma structures of the solar corona. These essentially compressive waves are confidently interpreted as slow magnetoacoustic waves. The use of the slow waves in plasma diagnostics and estimating their possible contribution to plasma heating and acceleration require detailed theoretical modelling. Aims. We investigate the role of obliqueness and magnetic effects in the evolution of slow magnetoacoustic waves, also called tube waves, in field-aligned plasma structures. Special attention is paid to the wave damping caused by nonlinear steepening. Methods. We considered an untwisted straight axisymmetric field-aligned plasma cylinder and analysed the behaviour of the slow magnetoacoustic waves that are guided by this plasma structure. We adopted a thin flux tube approximation. We took into account dissipation caused by viscosity, resistivity and thermal conduction, and nonlinearity. Effects of stratification and dispersion caused by the finite radius of the flux tube were neglected. Results. We derive the Burgers-type evolutionary equation for tube waves in a uniform plasma cylinder. Compared with a plane acoustic wave, the formation of shock fronts in tube waves is found to occur at a larger distance from the source. In addition, tube waves experience stronger damping. These effects are most pronounced in plasmas with the parameter beta at about or greater than unity. In a low-beta plasma, the evolution of tube waves can satisfactorily be described with the Burgers equation for plane acoustic waves.

Authors: A. N. Afanasyev, V.M. Nakariakov
Projects: None

Publication Status: A&A, accepted
Last Modified: 2014-11-03 07:57
Go to main E-Print page  On Polar Magnetic Field Reversal and Surface Flux Transport During Solar Cycle 24  Quasi-periodic pulsations in solar and stellar flares: re-evaluating their nature in the context of power-law flare Fourier spectra  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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