Geodesic
Dependence of the magnetic field generation models of in model of a $\alpha \Omega$-dynamo on the intensity of a power type $\alpha$-generator
Vestnik KRAUNC. Fiziko-matematičeskie nauki, Tome 29 (2019) no. 4, pp. 58-66 Cet article a éte moissonné depuis la source Math-Net.Ru

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In the dynamic model -dimensions are simulated reversions of the magnetic field with a varying intensity of the -generator. The change of the \alpha$-generator intensity as a result of synchronization of higher modes of the velocity field and the magnetic field is regulated by a function Z(t) with a power kernel. Dynamo modes are obtained for two types of radial component in the scalar parameterization of the $\alpha$-effect. The results were analyzed depending on the change in the exponent of the kernel of the function Z(t), also a comparative analysis with the results of the study [10], where the exponential kernel of the function Z(t) was used.
Keywords: large-scale dynamo model, $\alpha \Omega$-dynamo, magnetic field
Mots-clés : inversions. 
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     author = {A. N. Godomskaya and O. V. Sheremetyeva},
     title = {Dependence of the magnetic field generation models of in model of a $\alpha \Omega$-dynamo on the intensity of a power type $\alpha$-generator},
     journal = {Vestnik KRAUNC. Fiziko-matemati\v{c}eskie nauki},
     pages = {58--66},
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A. N. Godomskaya; O. V. Sheremetyeva. Dependence of the magnetic field generation models of in model of a $\alpha \Omega$-dynamo on the intensity of a power type $\alpha$-generator. Vestnik KRAUNC. Fiziko-matematičeskie nauki, Tome 29 (2019) no. 4, pp. 58-66. http://geodesic.mathdoc.fr/item/VKAM_2019_29_4_a6/

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