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Stationary flows in coronal loops
Authors:S Orlando  S Serio  G Peres
Institution:(1) Present address: Istituto ed Osservatorio Astronomico, Palermo;(2) Osservatorio Astrofisico di Catania, Catania, Italy;(3) Present address: IAIF, CNR Palermo, Palermo, Italy
Abstract:We present a study of stationary flows in closed solar coronal loops. The hydrodynamic differential equations of plasma flow and energy balance are integrated with algorithms which achieve high reliability. We present here results on the detailed synthesis of loop emission in specific bands and lines, taking into account also non-equilibrium ionization.
Keywords:Hydrodynamics  Loop Models  Solar Physics
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