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Three-dimensional simulations of near-surface convection in main-sequence stars - III. The structure of small-scale magnetic flux concentrations

MPS-Authors
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Beeck,  B.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

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Schüssler,  M.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Cameron,  R. H.
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Beeck, B., Schüssler, M., Cameron, R. H., & Reiners, A. (2015). Three-dimensional simulations of near-surface convection in main-sequence stars - III. The structure of small-scale magnetic flux concentrations. Astronomy and Astrophysics, 581: A42. doi:10.1051/0004-6361/201525788.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0028-FF02-B
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