Magnetic Structure of an Erupting Filament (2020)
Attributed to:
How do weak shocks accelerate high energy particles?
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/ab7380
Publication URI: http://dx.doi.org/10.3847/1538-4357/ab7380
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2