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

Details Magnetic field and differential rotation in the radiative zone of the sun Magnetic field and differential rotation in the radiative zone of the sun

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..142....1i&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 142, no. 1, p. 1-10.

Physics

4

Solar Interior, Solar Magnetic Field, Solar Rotation, Helioseismology, Solar Cycles, Solar Oscillations

Scientific paper

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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