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Study of the Coronal Heating in the Presence of Shear Flow: A Numerical Approach

Study of the Coronal Heating in the Presence of Shear Flow: A Numerical Approach

Goossens, M.; Tsurutani, B. T.
URI: http://hdl.handle.net/2014/22049
Date: 1997
Citation: USA

Abstract:

We numerically simulate the effect of shear flow on the evolution of MHD waves in the solar corona which is modeled by a low-beta, resistive plasma slab. The hydromagnetic waves are generated in the coronal loop by applying a periodic driver which mimics foot point motion in the photosphere.

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