A Dynamical Model for the Transition Zone and Inner Corona

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The authors investigate the effects of Alfven turbulence on a single magnetic tube by using a set of coupling equations of the flow-wave field in order to build up a dynamical model for the transition zone and inner corona. The calculations based on this dynamical model give results in basic agreement with obervations. Finally, the effect on the model through varying boundary condition is also dicussed.

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