Estimation of a coronal mass ejection magnetic field strength using radio observations of gyrosynchrotron radiation (2017)
Attributed to:
Consolidated Grant in Solar and Plasma Astrophysics
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201731368
Publication URI: http://dx.doi.org/10.1051/0004-6361/201731368
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics