Damping of Slow MHD Coronal Loop Oscillations by Shocks

Physics

Scientific paper

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Scientific paper

The damping of slow magnetoacoustic coronal loop oscillations by shock dissipation is investigated. Observations of large amplitude slow mode observations by SUMER show a clear dependency of the damping rate on the oscillation amplitude. Fully nonlinear MHD simulations of slow mode oscillations in the presence of thermal conduction are performed and the importance of various damping mechanisms a a function of amplitudes are investigated.

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