Coronal Holes and Open Magnetic Flux over Cycles 23 and 24
Abstract
As the observational signature of the footprints of solar magnetic field lines open into the heliosphere, coronal holes provide a critical measure of the structure and evolution of these lines. Using a combination of Solar and Heliospheric Observatory/Extreme ultraviolet Imaging Telescope (SOHO/EIT), Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA), and Solar Terrestrial Relations Observatory/Extreme Ultraviolet Imager...
Paper Details
Title
Coronal Holes and Open Magnetic Flux over Cycles 23 and 24
Published Date
Dec 27, 2016
Journal
Volume
292
Issue
1
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