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Velocity Shear Induced Phenomena in Solar Atmosphere
Authors:S. Poedts  A. D. Rogava  S. M. Mahajan
Affiliation:(1) Celestijnenlaan 200B, 3001 Heverlee, Belgium;(2) Inst. for Fusion Studies, The Univ. of Texas at Austin, Austin, TX 78712, USA
Abstract:We present a brief overview of the probable velocity-shear induced phenomena in solar plasma flows. Shear-driven MHD wave oscillations may be the needed mechanism for the generation of solar Alfvén waves, for the transmission of fast waves through the transition region, and for the acceleration of the solar wind. This revised version was published online in June 2006 with corrections to the Cover Date.
Keywords:shear flow  linear MHD  non-modal analysis
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