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The Sun Through Time
Magnetic activity of stars like the Sun evolves in time because of spin-down owing to angular momentum removal by a magnetized stellar wind. These magnetic fields are generated by an internal dynamo driven by convection and differential rotation. Spin-down therefore converges at an age of about 700 ...
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Springer Netherlands
2020
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7724955/ https://www.ncbi.nlm.nih.gov/pubmed/33328695 http://dx.doi.org/10.1007/s11214-020-00773-9 |