MHD wave motion in magnetically structured atmospheres

Details MHD wave motion in magnetically structured atmospheres MHD wave motion in magnetically structured atmospheres

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...119...28r&link_type=abstract

Astronomy and Astrophysics, vol. 119, no. 1, Mar. 1983, p. 28-34.

Physics

11

Magnetohydrodynamic Waves, Plasma Oscillations, Solar Atmosphere, Solar Magnetic Field, Transient Oscillations, Wave Propagation, Magnetic Flux, Magnetoacoustic Waves, Plasma Equilibrium, Solar Physics, Stable Oscillations, Wave Dispersion, Wave Fronts

Scientific paper

An examination of the MHD wave motions expected in magnetically structured regions of the solar atmosphere is completed using an idealised plane interface model. The steady-state solutions are characterised by wave energy fluxes possessing infinities when the equilibrium is at resonance. Under certain conditions wave energy is totally transmitted through magnetoacoustic boundaries. The transient solutions are characterised by a wave front trailing an oscillatory wake. A discussion of the predicted form of narrow-band solar MHD wave motions in magnetically structured regions is given.

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