The spatial damping of magnetohydrodynamic waves in a flowing partially ionised prominence plasma

Author： Carbonell M.   Forteza P.   Oliver R.   Ballester J. L.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|515|issue|A80-A80

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.515, Iss.issue, 2010-06, pp. : A80-A80

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Abstract

Context. Solar prominences are partially ionised plasmasdisplaying flows and oscillations. These oscillations exhibit timeand spatial damping and have commonly been explained in terms ofmagnetohydrodynamic (MHD) waves.

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