Convective overshoot and tachochlin are the most favorable the deep layers of the Sun to excite a toroidal magnetic field
The novelty of the models of the turbulent dynamo of the solar cycle, which were proposed in recent years, is that the generation of the poloidal and toroidal components of the global magnetic field does not occur equally effectively in the entire solar convective zone (SCZ), as was previously thoug...
| Main Author: | |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
National Aviation University
2018-12-01
|
| Series: | Вісник Астрономічної школи |
| Subjects: | |
| Online Access: | http://astro.nau.edu.ua/issues/2018_V.14_Iss.2/Krivodubskij.html |