Magnetic Fields in the Solar Convection Zone

Active regions on the solar surface are generally thought to originate from a strong toroidal magnetic field generated by a deep seated solar dynamo mechanism operating at the base of the solar convection zone. Thus the magnetic fields need to traverse the entire convection zone before they reach th...

Бүрэн тодорхойлолт

Номзүйн дэлгэрэнгүй
Үндсэн зохиолч: Yuhong Fan
Формат: Өгүүллэг
Хэл сонгох:English
Хэвлэсэн: Springer 2009-12-01
Цуврал:Living Reviews in Solar Physics
Нөхцлүүд:
Онлайн хандалт:http://www.livingreviews.org/lrsp-2009-4