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Estimation of a coronal mass ejection magnetic field strength using radio observations of gyrosynchrotron radiation (2017)

First Author: Carley E

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