Wave Heating of Coronal Loops with Steady Flows

摘要: We derive a general dispersion relation for hydromagnetic waves in inhomogeneous coronal loops with steady plasma flows. model static by assuming the equilibrium magnetic and configuration of solar as slab geometry, z-axis along uniform background field. assume density stratification perpendicular to direction Here we evaluate extent which can be collisionally dissipated, that is, their dissipation viscosity heat conduction when invoking flow, compare results minimum is required satisfy optically thin radiative cooling rate.