Evolution of the transverse density structure of oscillating coronal loops inferred by forward modelling of EUV intensity (2018)
Attributed to:
The Cool Alter-Ego of the Hot Solar Corona
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1808.03476
Publication URI: https://arxiv.org/abs/1808.03476
Type: Preprint