Abstract:С использованием асимптотического метода многих масштабов построена нелинейная теория возникновения крупномасштабных структур в стратифицированной проводящей среде при наличии мелкомасштабных осцилляций поля скорости и магнитных полей. Такие стационарные мелкомасштабные осцилляции поддерживаются малыми внешними источниками при ма лых числах Рейнольдса. Получена нелинейная система уравнений, описывающая эволюцию крупномасштабных структур поля скорости и магнитных полей. Линейная стадия эволюции приводит к извест… Show more
“…In the absence of heating ( =0) T and of external magnetic field ( = 0) B eqs. (27)-(28) coincide with the results found in [47]. In the case of non-electroconductive fluid ( = 0) with the temperature gradient ( 0) T we obtain the same results as in [50].…”
Section: Equations For Large-scale Fieldssupporting
confidence: 87%
“…(27)-(28) coincide with the results found in [47]. In the case of non-electroconductive fluid ( = 0) with the temperature gradient ( 0) T we obtain the same results as in [50]. In the limit of non-electroconductive ( = 0) and homogeneous fluid ( =0) T we obtain the results of [46].…”
Section: Equations For Large-scale Fieldssupporting
confidence: 85%
“…The development of this large-scale instability in obliquely rotating fluid gives rise to nonlinear large-scale helical structures of Beltrami vortex type, or to localized kinks with internal helical structure. In [47] the new hydrodynamic -effect found in [46] was generalized to the case of electroconductive fluid. The corresponding large-scale instability leads to the generation of LSVS and magnetic fields.…”
Section: Eejp 1 (2020)mentioning
confidence: 99%
“…This method allows to construct the nonlinear theories of vortex dynamo for compressible media [40][41], as well as for convective media with a helical external force [30][31]. The asymptotic multi-scale method is used to reveal large-scale instability in the thermally stratified conductive medium in the case of helicity of small-scale velocity and magnetic fields [42][43]. Development of this large-scale instability in a convective electroconductive medium engenders the generation of both vortex and magnetic fields as well.…”
Section: Eejp 1 (2020)mentioning
confidence: 99%
“…Development of this large-scale instability in a convective electroconductive medium engenders the generation of both vortex and magnetic fields as well. Self-consistent or nonlinear theory of magneto-vortex dynamo in a convective electroconductive medium with small-scale helicity was built in [43].…”
In this paper, we investigated a new large-scale instability that arises in an obliquely rotating convective electrically conducting fluid in an external uniform magnetic field with a small-scale external force with zero helicity. This force excites small-scale velocity oscillations with a small Reynolds number. Using the method of multiscale asymptotic expansions, we obtain the nonlinear equations for vortex and magnetic disturbances in the third order of the Reynolds number. It is shown that the combined effects of the Coriolis force and the small external forces in a rotating conducting fluid possible large-scale instability. The linear stage of the magneto-vortex dynamo arising as a result of instabilities of -effect type is investigated. The mechanism of amplification of large-scale vortex disturbances due to the development of the hydrodynamic - effect taking into account the temperature stratification of the medium is studied. It was shown that a «weak» external magnetic field contributes to the generation of large-scale vortex and magnetic perturbations, while a «strong» external magnetic field suppresses the generation of magnetic-vortex perturbations. Numerical methods have been used to find stationary solutions of the equations of a nonlinear magneto-vortex dynamo in the form of localized chaotic structures in two cases when there is no external uniform magnetic field and when it is present.
“…In the absence of heating ( =0) T and of external magnetic field ( = 0) B eqs. (27)-(28) coincide with the results found in [47]. In the case of non-electroconductive fluid ( = 0) with the temperature gradient ( 0) T we obtain the same results as in [50].…”
Section: Equations For Large-scale Fieldssupporting
confidence: 87%
“…(27)-(28) coincide with the results found in [47]. In the case of non-electroconductive fluid ( = 0) with the temperature gradient ( 0) T we obtain the same results as in [50]. In the limit of non-electroconductive ( = 0) and homogeneous fluid ( =0) T we obtain the results of [46].…”
Section: Equations For Large-scale Fieldssupporting
confidence: 85%
“…The development of this large-scale instability in obliquely rotating fluid gives rise to nonlinear large-scale helical structures of Beltrami vortex type, or to localized kinks with internal helical structure. In [47] the new hydrodynamic -effect found in [46] was generalized to the case of electroconductive fluid. The corresponding large-scale instability leads to the generation of LSVS and magnetic fields.…”
Section: Eejp 1 (2020)mentioning
confidence: 99%
“…This method allows to construct the nonlinear theories of vortex dynamo for compressible media [40][41], as well as for convective media with a helical external force [30][31]. The asymptotic multi-scale method is used to reveal large-scale instability in the thermally stratified conductive medium in the case of helicity of small-scale velocity and magnetic fields [42][43]. Development of this large-scale instability in a convective electroconductive medium engenders the generation of both vortex and magnetic fields as well.…”
Section: Eejp 1 (2020)mentioning
confidence: 99%
“…Development of this large-scale instability in a convective electroconductive medium engenders the generation of both vortex and magnetic fields as well. Self-consistent or nonlinear theory of magneto-vortex dynamo in a convective electroconductive medium with small-scale helicity was built in [43].…”
In this paper, we investigated a new large-scale instability that arises in an obliquely rotating convective electrically conducting fluid in an external uniform magnetic field with a small-scale external force with zero helicity. This force excites small-scale velocity oscillations with a small Reynolds number. Using the method of multiscale asymptotic expansions, we obtain the nonlinear equations for vortex and magnetic disturbances in the third order of the Reynolds number. It is shown that the combined effects of the Coriolis force and the small external forces in a rotating conducting fluid possible large-scale instability. The linear stage of the magneto-vortex dynamo arising as a result of instabilities of -effect type is investigated. The mechanism of amplification of large-scale vortex disturbances due to the development of the hydrodynamic - effect taking into account the temperature stratification of the medium is studied. It was shown that a «weak» external magnetic field contributes to the generation of large-scale vortex and magnetic perturbations, while a «strong» external magnetic field suppresses the generation of magnetic-vortex perturbations. Numerical methods have been used to find stationary solutions of the equations of a nonlinear magneto-vortex dynamo in the form of localized chaotic structures in two cases when there is no external uniform magnetic field and when it is present.
This paper presents the results of numerical investigation, calculation analysis and experimental study of heat exchange in a system of plane-parallel channels formed by rectangular fins, which are applied in a heat removal device using heat tubes for power semiconductor energy converters. Passive cooling (heat removal by radiation and natural convection) and active cooling (heat removal by radiation and forced convection) are investigated for various velocities of air cooling of fins by spherical vortex generators applied to its surface. A comparative analysis of the results is carried out for the average effective heat removal resistance and for the average temperature at the ends of the fins. The application of numerical modeling to solve such problems confirms the effectiveness of computational technologies. The difference between the results of the study ranges from 10 to 16% depending on the airflow rate.
The survey covers a main achievements in the field of dynamo theory. Applications of the model of turbulent convective dynamo to the problem of generation of a large-scale vortexes and magnetic structures in the solar photosphere are discussed. Investigated are the new models of the vortex dynamo in a rotating fluid with small-scale external force. The main results in these models are obtained by the method of multiscale asymptotic expansions. The results of numerical analysis of nonlinear equations of a magnetovortex dynamo in a stationary mode are provided. Solutions are found in the form of spiral kinks, periodic nonlinear waves and solitons, which are also considered in the survey.
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