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Paper: Alfvén Wave Dynamics in the Expanding Solar Corona
Volume: 463, 2nd ATST-EAST Workshop in Solar Physics: Magnetic Fields from the Photosphere to the Corona
Page: 175
Authors: Kaghashvili, E. Kh.
Abstract: We investigate the evolution of the linearly polarized Alfvén wave in the magnetic field-aligned flow. The main focus is a temporal interface during which the Alfvén wave transitions from the almost zero cross-shear flow of the lower solar atmosphere to the expanding solar corona region. A possible link between our numerical simulations and the detected coronal intensity fluctuations is discussed.
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