Diagnostics of Non-Maxwellian Electron Distributions in Solar Active Regions from Fe xii Lines Observed by the Hinode Extreme Ultraviolet Imaging Spectrometer and Interface Region Imaging Spectrograph (2022)
Attributed to:
UNDERSTANDING THE DYNAMICAL SOLAR ATMOSPHERE
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/ac6174
Publication URI: http://dx.doi.org/10.3847/1538-4357/ac6174
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1