An empirical 3D model of the large-scale coronal structure based on the distribution of Hα filaments on the solar disk
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20066482/pdf
Reference41 articles.
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4. Time–Latitudinal Development of the White-Light Coronal Structures over a Solar Cycle
5. Multiple heliospheric current sheets and coronal streamer belt dynamics
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