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An Analysis of the Solar Rotation Velocity by Tracing Coronal Features
Published online by Cambridge University Press: 13 May 2016
Abstract
The solar rotation is determined tracing coronal EUV and soft X-ray bright points, active regions, parts of coronal holes and foot points of coronal loops. Full-disc solar images in the EUV part of the spectrum from the SOHO spacecraft (EIT, Fe XV, 28.4 nm) and from the Yohkoh satellite (SXT, 2 nm) are used.
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- Session IV: Structure and Dynamics of the Transiton Region and Corona
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- Copyright © Astronomical Society of the Pacific 2001
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