Sausage Mode Propagation in a Thick Magnetic Flux Tube

The aim of this paper is to model the propagation of slow magnetohydrodynamic (MHD) sausage waves in a thick expanding magnetic flux tube in the context of the quiescent (VAL-C) solar atmosphere. The propagation of these waves is found to be described by the Klein–Gordon equation. Using the governin...

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Veröffentlicht in:Solar physics 2014-04, Vol.289 (4), p.1203-1214
Hauptverfasser: Pardi, A., Ballai, I., Marcu, A., Orza, B.
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creator Pardi, A.
Ballai, I.
Marcu, A.
Orza, B.
description The aim of this paper is to model the propagation of slow magnetohydrodynamic (MHD) sausage waves in a thick expanding magnetic flux tube in the context of the quiescent (VAL-C) solar atmosphere. The propagation of these waves is found to be described by the Klein–Gordon equation. Using the governing MHD equations and the VAL-C atmosphere model we study the variation of the cut-off frequency along and across the magnetic tube guiding the waves. Due to the radial variation of the cut-off frequency the flux tubes act as low frequency filters for the waves.
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source Springer Nature - Complete Springer Journals
subjects Astrophysics and Astroparticles
Atmosphere
Atmospheric Sciences
Fluctuations
Physics
Physics and Astronomy
Solar physics
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
Waves
title Sausage Mode Propagation in a Thick Magnetic Flux Tube
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