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/10.17863/cam.68684
Publication URI: https://www.repository.cam.ac.uk/handle/1810/321564
Type: Journal Article/Review