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Cited by 189

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Stellar evolution with rotation and magnetic fields: IV. The solar rotation profile

Open access
Eggenberger, P., Maeder, A., Meynet, G.·2005·Astronomy & Astrophysics
DOI 10.1051/0004-6361:200500156
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Abstract

We examine the generation of a magnetic field in a solar-like star and its effects on the internal distribution of the angular velocity. We suggest that the evolution of a rotating star with magnetic fields leads to an equilibrium value of the differential rotation. This equilibrium is determined by the magnetic coupling, which favours a constant rotation profile, and meridional circulation which tends to build differential rotation. The global equilibrium stage is close to solid body rotation between about 0.7 and 0.2 , in good agreement with helioseismic measurements.

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Metadata

Authors
Eggenberger, P., Maeder, A., & Meynet, G.
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2005-08-19
Volume
440
Issue
1
Pages
L9-L12
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
DOI
10.1051/0004-6361:200500156
OpenAlex
W4293713796
Cited by
189
References
0
FWCI
6.25
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Stellar evolution with rotation and magnetic fields: IV. The solar rotation profile. https://app.cochat.ai/papers/10.1051/0004-6361:200500156
The paper
Eggenberger, P., Maeder, A., & Meynet, G. (2005). Stellar evolution with rotation and magnetic fields: IV. The solar rotation profile. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A200500156

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.