A new trigger mechanism for coronal mass ejections: the role of confined flares and photospheric motions in the formation of hot flux ropes (2020)
Attributed to:
MSSL Solar & Planetary Physics Consolidated Grant 2016-2019
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2010.11204
Publication URI: https://arxiv.org/abs/2010.11204
Type: Other