Flare Kernels May be Smaller than You Think: Modelling the Radiative Response of Chromospheric Plasma Adjacent to a Solar Flare (2022)
Attributed to:
Consolidated Grant in Solar Physics
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2209.03238
Publication URI: https://arxiv.org/abs/2209.03238
Type: Other