Issue |
A&A
Volume 642, October 2020
|
|
---|---|---|
Article Number | C2 | |
Number of page(s) | 1 | |
Section | The Sun and the Heliosphere | |
DOI | https://doi.org/10.1051/0004-6361/202037739e | |
Published online | 20 October 2020 |
How faculae and network relate to sunspots, and the implications for solar and stellar brightness variations(Corrigendum)
1
Max-Planck Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany
e-mail: yeo@mps.mpg.de
2
School of Space Research, Kyung Hee University, Yongin, 446-701 Gyeonggi, Korea
This article has no abstract.
Key words: Sun: activity / Sun: faculae, plages / Sun: magnetic fields / sunspots / errata, addenda
© K. L. Yeo et al. 2020
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.
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.