๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Magnetic field and differential rotation in the radiative zone of the Sun

โœ Scribed by R. N. Ikshanov; V. G. Ivanov

Publisher
Springer
Year
1992
Tongue
English
Weight
554 KB
Volume
142
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

The problem of the interaction between magnetic fields and differential rotation in the radiative zone of the Sun is investigated. It is demonstrated that effects of magnetic buoyancy can be neglected in the analysis of this interaction. It is shown that hydromagnetic torsional waves propagating from the solar core cannot be responsible for the 22-year solar cycle. A possible geometry of the magnetic field that conforms with stationary differential rotation is considered. A verifying method for hypotheses on the structure of the magnetic field and torsional oscillations in the radiative zone of the Sun is proposed based on helioseismic data.

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