Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...305..977c&link_type=abstract
Astronomy and Astrophysics, v.305, p.977
Astronomy and Astrophysics
Astrophysics
12
Sun: Corona, Sun: Magnetic Fields, Magnetohydrodynamics
Scientific paper
We consider an isolated potential magnetic arcade with a thick boundary forming a layer with strongly nonpotential field, that separates the interior of the arcade from the ambient nonmagnetized plasma of the solar corona. It is shown that, in this case, local surface waves, having a relatively large wavelength compared to the layer thickness, can resonantly generate a continuous MHD slow mode spectrum within the layer. The obtained rate coefficient depends on the value of the field gradient at the place where the resonance occurs and it vanishes when the gradient tends to infinity.
Ballester Jose Luis
Cadez Vladimir M.
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