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CORONAL ALFVÉN SPEED DETERMINATION: CONSISTENCY BETWEEN SEISMOLOGY USING AIA/SDOTRANSVERSE LOOP OSCILLATIONS AND MAGNETIC EXTRAPOLATION

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STANDING SAUSAGE MODES IN NONUNIFORM MAGNETIC TUBES: AN INVERSION SCHEME FOR INFERRING FLARE LOOP PARAMETERS

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Mixed Properties of MHD Waves in Non-uniform Plasmas

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Damping of Fast Magnetohydrodynamic Oscillations in Quiescent Filament Threads

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Inference of magnetic field strength and density from damped transverse coronal waves

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No unique solution to the seismological problem of standing kink magnetohydrodynamic waves

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