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- W1809366959 abstract "It is conjectured that a magnetic field in the convective envelopes of stars compensates a mean azimutal force, which is equivalent to negative viscosity, produced by the convective motions. Some examples confirm the existence of such a negative viscosity effect. According to the conjecture, the azimuthal force not only maintains the differential rotation of the medium but also draws out the lines of force of the field, producing a toroidal from a poloidal field. It is assumed that the direction of the poloidal field component reverses at the end of the enhancement stage in a certain layer situated below the main zone of the enhancement of the field. The reversal of the field direction is attributed to an instability (however, this process needs further study). (AIP)" @default.
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- W1809366959 title "Possible mechanism of the solar cycle" @default.
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