| 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
Key words: Sun: activity / Sun: faculae, plages / Sun: magnetic fields / sunspots / errata, addenda
This is a corrigendum to Yeo et al. (2020). We had listed the wrong values for the parameter h1 in Table 1. The error is purely typographical and confined to this table, and as such there is no impact on the rest of the paper. The revised table is given below.
Similar to Table 1 in Yeo et al. (2020), except with the correct values of h 1.
References
- Yeo, K. L., Solanki, S. K., & Krivova, N. A. 2020, A&A, 639, A139 [CrossRef] [EDP Sciences] [Google Scholar]
© 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.
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