Issue |
A&A
Volume 677, September 2023
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 1 | |
Section | Stellar atmospheres | |
DOI | https://doi.org/10.1051/0004-6361/202243607e | |
Published online | 29 August 2023 |
Small-scale dynamo in cool stars
I. Changes in stratification and near-surface convection for main-sequence spectral types (Corrigendum)
1
Max-Planck-Institut für Sonnensystemforschung,
Justus-von-Liebig Weg 3,
37077
Göttingen,
Germany
e-mail: bhatia@mps.mpg.de
2
School of Space Research, Kyung Hee University, Yongin,
Gyeonggi-Do
446-701,
Korea
Key words: stars: interiors / stars: late-type / stars: magnetic field / convection / dynamo / errata, addenda
The derivation in Appendix B of the original paper contains a typo. The result is however correct, and the typo does not otherwise affect the paper. The first line in the right-hand column on page 9 should have read “The pressure balance along the vertical (z) direction involves the term 〈∇i · σiz〉z which is equal to ∂Ptot/∂z.” Here, summation over i is implied. The original sentence inadvertently had 〈∇z · σiz〉z. The result then follows trivially from the fundamental theorem of calculus, and the periodicity of B in the horizontal direction, which implies .
© The Authors 2023
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.
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Open Access funding provided by Max Planck Society.
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