Issue |
A&A
Volume 669, January 2023
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 2 | |
Section | The Sun and the Heliosphere | |
DOI | https://doi.org/10.1051/0004-6361/202141451e | |
Published online | 22 December 2022 |
A solar coronal loop in a box: Energy generationand heating (Corrigendum)
1
Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany
e-mail: breu@mps.mpg.de
2
School of Space Research, Kyung Hee University, Yongin, Gyeonggi 446-701, Republic of Korea
3
High Altitude Observatory, NCAR, P.O. Box 3000, Boulder, Colorado 80307, USA
This article has no abstract.
Key words: Sun: corona / Sun: magnetic fields / magnetohydrodynamics (MHD) / errata, addenda
© The Authors 2022
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
This article is published in open access under the Subscribe-to-Open model.
Open Access funding provided by Max Planck Society.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.