Observations of Cool-Star Magnetic Fields
Cool stars like the Sun harbor convection zones capable of producing substantial surface magnetic fields leading to stellar magnetic activity. The influence of stellar parameters like rotation, radius, and age on cool-star magnetism, and the importance of the shear layer between a radiative core and...
| Auteur principal: | |
|---|---|
| Format: | Article |
| Langue: | English |
| Publié: |
Springer
2012-02-01
|
| Collection: | Living Reviews in Solar Physics |
| Sujets: | |
| Accès en ligne: | http://www.livingreviews.org/lrsp-2012-1 |