The connection between stellar activity cycles and magnetic field topology

Zeeman–Doppler imaging (ZDI) has successfully mapped the large-scale magnetic fields of stars over a large range of spectral types, rotation periods and ages. When observed over multiple epochs, some stars show polarity reversals in their global magnetic fields. On the Sun, polarity reversals are a...

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Principais autores: See, V., Jardine, M., Vidotto, A. A., Donati, J. F., Saikia, S. Boro, Bouvier, J., Fares, R., Folsom, C. P., Gregory, S. G., Hussain, G., Jeffers, S. V., Marsden, S. C., Morin, J., Moutou, C., Nascimento Júnior, José Dias do, Petit, P., Waite, I. A.
Formato: article
Idioma:pt_BR
Publicado: Royal Astronomical Society
Assuntos:
Techniques - polarimetric
Stars - activity
Stars - evolution
Stars - magnetic field
Stars - rotation
Acceso en liña:https://repositorio.ufrn.br/jspui/handle/123456789/29046
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https://repositorio.ufrn.br/jspui/handle/123456789/29046

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