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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

V. N. Kryvodubskyj
V. N. Kryvodubskyj*
Affiliation:
Astronomical Observatory of Kyiv National University Observatorna Street 3, Kyiv − 53, 04053, Ukraine

Abstract

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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
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 118 - 120
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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