Non-thermal broadening of IRIS Fe XXI line caused by turbulent plasma flows in the magnetic reconnection region during solar eruptions (2023)
Attributed to:
Post-launch Support for UK continued involvement in the Japanese Hinode Mission
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3389/fspas.2023.1096133
Publication URI: http://dx.doi.org/10.3389/fspas.2023.1096133
Type: Journal Article/Review
Parent Publication: Frontiers in Astronomy and Space Sciences