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arXiv · 0806.1418

Magneto-Acoustic Wave Oscillations in Solar Spicules

Abstract

Some observations suggest that solar spicules show small amplitude and high frequency oscillations of magneto-acoustic waves, which arise from photospheric granular forcing. We apply the method of MHD seismology to determine the period of kink waves. For this purposes, the oscillations of a magnetic cylinder embedded in a field-free environment is investigated. Finally, diagnostic diagrams displaying the oscillatory period in terms of some equilibrium parameters are provided to allow a comparison between theoretical results and those coming from observations.

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BibTeXRIS

A. Ajabshirizadeh, E. Tavabi, S. Koutchmy. 2008-06-09. Magneto-Acoustic Wave Oscillations in Solar Spicules. https://doi.org/10.1007/s10509-008-9951-z

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