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Quadrupole Mode of the Sun's Poloidal Magnetic Field: on the Possibility of Exciting by Turbulent Dynamo Mechanism
Published online by Cambridge University Press: 13 May 2016
Abstract
On the base of turbulent dynamo model with allowance for newer helioseismic measurements of the Sun's inner rotation it is shown that the physical conditions in deep layers of the solar convection zone in near-pole domain are favourable for exciting of quadrupole mode of poloidal magnetic field near maximum phase of 23-rd solar cycle
- Type
- Session I: Global Structure and Evolution of the Solar Interior
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- Copyright © Astronomical Society of the Pacific 2001