Intermittence and peculiarities of a statistic characteristic of the geomagnetic field in geodynamo models
- Авторы: Khokhlov A.V.1,2, Lhuillier F.3, Shcherbakov V.P.2,4,5
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Учреждения:
- Institute of Earthquake Prediction Theory and Mathematical Geophysics
- Schmidt Institute of Physics of the Earth
- Ludwig-Maximilian University of Munich
- Kazan (Volga Region) Federal University
- Borok Geophysical Observatory, Schmidt Institute of Physics of the Earth
- Выпуск: Том 53, № 5 (2017)
- Страницы: 695-701
- Раздел: Article
- URL: https://journals.rcsi.science/1069-3513/article/view/224215
- DOI: https://doi.org/10.1134/S106935131705007X
- ID: 224215
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Аннотация
The analysis of the statistical characteristics of the geomagnetic field generated in the numerical geodynamo models has shown that the distribution of the spherical harmonic coefficients in some cases is not Gaussian but, instead, has much in common with the Laplace distribution. The shape of the corresponding histograms depends on the time scale, which allows interpreting the obtained data in terms of a mixture of Gaussian distributions. The similar effects associated with the intermittence were observed in the experiments in a turbulent fluid flow. Hence, the behavior of secular variations in the magnetic field of the Earth should perhaps be described in terms of a mixture of several Gaussian stationary processes corresponding to switching between the different regimes of geodynamo generation.
Об авторах
A. Khokhlov
Institute of Earthquake Prediction Theory and Mathematical Geophysics; Schmidt Institute of Physics of the Earth
Автор, ответственный за переписку.
Email: fbmotion@yandex.ru
Россия, Moscow, 117997; Moscow, 123995
F. Lhuillier
Ludwig-Maximilian University of Munich
Email: fbmotion@yandex.ru
Германия, Munich
V. Shcherbakov
Schmidt Institute of Physics of the Earth; Kazan (Volga Region) Federal University; Borok Geophysical Observatory, Schmidt Institute of Physics of the Earth
Email: fbmotion@yandex.ru
Россия, Moscow, 123995; Kazan, 420111; Borok, 152742
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