[https://doi.org/10.1051/0004-6361/202142996]
[https://doi.org/10.1051/0004-6361/201834154]
Issue |
A&A
Volume 683, March 2024
|
|
---|---|---|
Article Number | C2 | |
Number of page(s) | 1 | |
Section | The Sun and the Heliosphere | |
DOI | https://doi.org/10.1051/0004-6361/202449183e | |
Published online | 11 March 2024 |
Magnetic field amplification and structure formation by the Rayleigh-Taylor instability (Corrigendum)
1
Centre for mathematical Plasma Astrophysics, KU Leuven, 3001 Leuven, Belgium
e-mail: beatriceannemone.popescubraileanu@kuleuven.be
2
Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain
3
Departamento de Astrofísica, Universidad de La Laguna, 38205 La Laguna, Tenerife, Spain
4
National Science Foundation, Alexandria, VA 22306, USA
Key words: magnetic reconnection / Sun: magnetic fields / Sun: filaments / prominences / instabilities / errata / addenda
There were some errors, which do not affect the results that were presented, in the expressions for the viscosity and thermal conductivity coefficients and cross sections. The correct ones, that is to say those used in the code in all of the simulations, are as follows:
The collisional cross sections used in Eqs. (1) and (2) are
The incorrect expressions appear in the following:
-
Eq. (12) in Popescu Braileanu et al. (2023),
-
Eq. (A.10) in Popescu Braileanu et al. (2019).
References
- Popescu Braileanu, B., Lukin, V. S., Khomenko, E., & de Vicente, Á. 2019, A&A, 627, A25 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Popescu Braileanu, B., Lukin, V. S., & Khomenko, E. 2023, A&A, 670, A31 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© The Authors 2024
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