Alfvén waves, made to propagate along an ambient magnetic field and polarized transverse to a gravitational field , with wave amplitude stratified along , are shown to reduce the growth rate of interchange instability by increasing the effective inertia by a factor of , where is the ambient magnetic field, is the wavenumber, and is the wave amplitude shear. Appropriately placed Alfvén wave power could thus be used to enhance the stability of interchange and ballooning modes in tokamaks and other interchange-limited magnetically confined plasmas.
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