Zonal latitude structure of the Sun's global magnetic field excited by turbulent dynamo mechanism

Details Zonal latitude structure of the Sun's global magnetic field excited by turbulent dynamo mechanism Zonal latitude structure of the Sun's global magnetic field excited by turbulent dynamo mechanism

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..451k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 451-452

Physics

Scientific paper

This study is performed on the base of the turbulent dynamo model allowed newer helioseismic measurements of the Sun's inner rotation. It is shown that the physical conditions in the deep layers of the solar convection zone in the near-pole domain are favourable for exciting of quadrupole mode of the poloidal magnetic field near maximum phase of the 23rd solar cycle.

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