Modeling of the magnetic field polarity reversal processes in planets and stars.

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Magnetic Fields: Magnetohydrodynamics

Scientific paper

A possibility of implementing the conditions of magnetic field freezing by the materials possessing permanent magnetism has been demonstrated experimentally. A condition that supports the magnetic field by the MHD dynamo mechanism is the motion wherein one neighboring force line of the field slides along another. Several hypotheses explain the polarity reversal of the magnetic field by the instability of a turbulent M-profile of the different rotation velocities in the liquid metal core of the planets and emphasize two types of convective flow: a turbulent one in the liquid metal core and a laminar one in the outside semiliquid zone, i.e., the asthenosphere, as the sources of the total magnetic field of the Earth.

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