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This article is cited in 2 scientific papers (total in 2 papers)
MATHEMATICAL MODELING
Dependence of the magnetic field generation models of in model of a $\alpha \Omega$-dynamo on the intensity of a power type $\alpha$-generator
A. N. Godomskayaa, O. V. Sheremetyevab a Municipal Budgetary Institution for Supplementary Education Center Luch , 684000, Elizovo, Timiryazevsky Lane, 9, Russia
b Institute of Cosmophysical Researches and RadioWave Propagation Far-Eastern Branch, Russian Academy of Sciences, 684034, Kamchatskiy Kray, Paratunka, Mirnaya st., 7, Russia
Abstract:
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, inversions.
Citation:
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. Fiz.-Mat. Nauki, 29:4 (2019), 58–66
Linking options:
https://www.mathnet.ru/eng/vkam370 https://www.mathnet.ru/eng/vkam/v29/i4/p58
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