Angular momentum transport by MHD turbulence and torsional oscillations of the sun

Details Angular momentum transport by MHD turbulence and torsional oscillations of the sun Angular momentum transport by MHD turbulence and torsional oscillations of the sun

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..652k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, July 1990, p. 652-660. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Angular Momentum, Magnetohydrodynamic Turbulence, Momentum Transfer, Solar Magnetic Field, Solar Oscillations, Magnetic Field Configurations, Solar Rotation, Torsion

Scientific paper

Magnetic fields are shown to produce qualitative changes of the sources of solar differential rotation rather than quenching them, as is usually assumed. Additional equatorward flux of angular momentum arises under the influence of toroidal magnetic fields. The possibility of interpreting the torsional oscillations of the sun as a result of magnetic-field influence on turbulent angular-momentum fluxes is discussed.

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