Can We Detect Coronal Mass Ejections through Asymmetries of Sun-as-a-star Extreme-ultraviolet Spectral Line Profiles? (2022)
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/10.3847/1538-4365/ac6607
Publication URI: http://dx.doi.org/10.3847/1538-4365/ac6607
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal Supplement Series
Issue: 2