Meridional motions and Reynolds stress from SDO/AIA coronal bright points data⋆

Author： Sudar D.   Saar S. H.   Skokić I.   Poljančić Beljan I.   Brajša R.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|587|issue|A29-A29

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.587, Iss.issue, 2016-02, pp. : A29-A29

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Abstract

Context. It is possible to detect and track coronal bright points (CBPs) in Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) images. A combination of high resolution and high cadence provides a wealth of data that can be used to determine velocity flows on the solar surface with very high accuracy.

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