A New Parameter of the Photospheric Magnetic Field to Distinguish Eruptive-flare Producing Solar Active Regions
Author:
Funder
MEXT/JSPS KAKENHI
US National Science Foundation
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab822c/pdf
Reference60 articles.
1. Magnetic fields and the structure of the solar corona
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