In 2D MHD simulations of solar filament longitudinal oscillations with gravity comparable to the Lorentz force, wave leakage and non-adiabatic losses shorten the decay time and make the pendulum model's curvature estimate about 100 percent off.
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Damping Mechanisms of the Solar Filament Longitudinal Oscillations in Weak Magnetic Field
In 2D MHD simulations of solar filament longitudinal oscillations with gravity comparable to the Lorentz force, wave leakage and non-adiabatic losses shorten the decay time and make the pendulum model's curvature estimate about 100 percent off.