High Resolution Soft X-ray Spectroscopy and the Quest for the Hot (5-10 MK) Plasma in Solar Active Regions (2021)
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/10.3389/fspas.2021.638489
Publication URI: http://dx.doi.org/10.3389/fspas.2021.638489
Type: Journal Article/Review
Parent Publication: Frontiers in Astronomy and Space Sciences