Automated Identification of Coronal Holes from Synoptic EUV Maps
Abstract
Coronal holes (CHs) are regions of open magnetic field lines in the solar corona and the source of the fast solar wind. Understanding the evolution of coronal holes is critical for solar magnetism as well as for accurate space weather forecasts. We study the extreme ultraviolet (EUV) synoptic maps at three wavelengths (195 Å/193 Å, 171 Å and 304 Å) measured by the Solar and Heliospheric Observatory/Extreme Ultraviolet Imaging Telescope...
Paper Details
Title
Automated Identification of Coronal Holes from Synoptic EUV Maps
Published Date
Apr 1, 2018
Journal
Volume
293
Issue
4
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