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/10.48550/arxiv.1601.07308
Publication URI: https://arxiv.org/abs/1601.07308
Type: Other