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Stationary large-scale magnetic fields generated by turbulent motion in a spherical region (1996)

Yoshizawa, Akira ; Yokoi, Nobumitsu

[S.l.] : American Institute of Physics (AIP)

Physics of Plasmas 3 (1996), S. 3604-3613

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ISSN: 1089-7674

Source: AIP Digital Archive

Topics: Physics

Notes: Stationary large-scale magnetic fields generated by an electrically conducting fluid in a spherical region are examined analytically, using the concept of the turbulent dynamo based on helicity and cross-helicity effects. Under this concept, the toroidal magnetic field is induced through the combination of a rotational motion and the turbulent cross-helicity effect. This field generates the poloidal one through the turbulent residual-helicity (alpha) effect. A new magnetic-field generation mechanism in the vicinity of the poles is also described. These findings are discussed in the context of the dimension of the convection part of a stellar object. © 1996 American Institute of Physics.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1063/1.871952

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