Non-Maxwellian Analysis of the Transition-region Line Profiles Observed by the Interface Region Imaging Spectrograph (2017)
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/aa71a8
Publication URI: http://dx.doi.org/10.3847/1538-4357/aa71a8
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1