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Small-scale EUV features as the drivers of coronal upflows in the quiet Sun (2023)

First Author: Schwanitz C

Attributed to: How do weak shocks accelerate high energy particles? funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202346036

Publication URI: http://dx.doi.org/10.1051/0004-6361/202346036

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics