Coronal Holes and Open Magnetic Flux over Cycles 23 and 24

Volume: 292, Issue: 1
Published: Dec 27, 2016
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
Volume
292
Issue
1
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