Magnetic Structures at the Boundary of the Closed Corona: Interpretation of S-Web Arcs (2018)
Attributed to:
Dynamics of Complex Magnetic Fields: From the corona to the solar wind
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aaed2b
Publication URI: http://dx.doi.org/10.3847/1538-4357/aaed2b
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1