First evidence of non-Gaussian solar flare EUV spectral line profiles and accelerated non-thermal ion motion (2016)
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/10.1051/0004-6361/201527986
Publication URI: http://dx.doi.org/10.1051/0004-6361/201527986
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics