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Internal Large-Scale Toroidal Magnetic Field of the Sun

Published online by Cambridge University Press:  19 July 2016

V.N. Krivodubskij*
Affiliation:
Kiev Shevchenko University Astronomical Observatory Observatornaya Street, 3 Kiev - 53, 252053 Ukraine, U.S.S.R.

Extract

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The evolution of the large-scale toroidal magnetic field Bϕ of the Sun generating in the radiative zone by acts of differential rotation on the relict radial magnetic field Bϕ is investigated regarding the magnetic buoyancy and ohmic dissipation.

Type
II. The Solar Interior
Copyright
Copyright © Kluwer 1990