MHD Waves in Coronal Loops: The Effects of the Surrounding Corona

Details MHD Waves in Coronal Loops: The Effects of the Surrounding Corona MHD Waves in Coronal Loops: The Effects of the Surrounding Corona

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996plas.work..154o&link_type=abstract

Proceedings of the Fourth Brazilian Meeting on Plasma Physics and the Sixth Brazilian Plasma Astrophysics Workshop, p. 154

Physics

Plasma Physics

Magnetohydrodynamic Waves, Magnetohydrodynamics, Magnetic Flux, Magnetoacoustics, Continuums, Spectrum Analysis, Oscillations, Coronas, Coronal Loops

Scientific paper

We present the ideal magnetohydrodynamic (MHD) spectral analysis of a two-layered magnetic flux tube with model parameters which represent a typical coronal loop surrounded by the ambient corona. Alfven surface modes concentrated at the loop - corona interface are not expected to appear due to the absence of a gap between the two branches of the Alfven continuum. Fast magnetosonic modes are found, corresponding to oscillations of the order of a few seconds.

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