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High resolution soft X-ray spectroscopy and the quest for the hot (5-10 MK) plasma in solar active regions (2021)

First Author: Del Zanna G

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/10.48550/arxiv.2103.06156

Publication URI: https://arxiv.org/abs/2103.06156

Type: Preprint