Path-lengths in the quiet Sun transition region using O iv lines from IRIS (2022)
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/10.1093/mnras/stac2772
Publication URI: http://dx.doi.org/10.1093/mnras/stac2772
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1