Small-scale Turbulent Motion of the Plasma in a Solar Filament as the Precursor of Eruption (2021)
Attributed to:
Understanding the chromosphere-corona interface in the Solar Orbiter and DKIST era
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2106.11875
Publication URI: https://arxiv.org/abs/2106.11875
Type: Other