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pro vyhledávání: '"Sergey V. Starchenko"'
Publikováno v:
Springer Proceedings in Earth and Environmental Sciences ISBN: 9783030914660
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d7ca97afe355b8da123a5cee09cf09ae
https://doi.org/10.1007/978-3-030-91467-7_16
https://doi.org/10.1007/978-3-030-91467-7_16
Publikováno v:
Springer Proceedings in Earth and Environmental Sciences ISBN: 9783030914660
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8c77bdc33134dddb4f6fa02ffa9ba397
https://doi.org/10.1007/978-3-030-91467-7_15
https://doi.org/10.1007/978-3-030-91467-7_15
Autor:
Sergey V. Starchenko
Publikováno v:
Geophysical & Astrophysical Fluid Dynamics. 113:71-79
Numerical models of planetary MHD dynamos have led to many advances in the last twenty years. However, the accessible parameter space of these models is somewhat limited due to computational constr...
Publikováno v:
Journal of Fluid Mechanics. 689:376-416
A Boussinesq fluid of kinematic velocity$\nu $and thermal diffusivity$\kappa $is confined within a rapidly rotating shell with inner and outer sphere boundary radii${ r}_{i}^{\ensuremath{\ast} } $and${ r}_{o}^{\ensuremath{\ast} } $, respectively. The
Publikováno v:
Geophysical & Astrophysical Fluid Dynamics. 100:397-427
Almost adiabatic states are typical for the deep convective interiors of all known planets and their moons, e.g., the deviations from the adiabatic state in the Earth's outer core and in the MHD dynamo region of Jupiter are about or less than 10−5%
Autor:
Sergey V. Starchenko
Publikováno v:
Physics of Fluids. 10:2412-2420
We consider the motion of a spherical annulus of fluid driven by the slightly differential rotation of the confining spherical shells. The novelty of our analysis is the imposition of a strong axisymmetric potential magnetic field on a conducting ann
Autor:
Sergey V. Starchenko, Masaru Kono
Publikováno v:
Geophysical & Astrophysical Fluid Dynamics. 82:93-123
The Maximally Efficient Generation Approach (MEGA) is a method to find approximate solutions in a region where strong differential rotation (ω-effect) and helicity (α-effect) coexist (Ruzmaikin et ...
Autor:
Sergey V. Starchenko
Publikováno v:
Geophysical & Astrophysical Fluid Dynamics. 77:55-77
Suggested approximation of a strong generation reduces the kinematic dynamo problem to one simple scalar equation which has a local analytical solution near the maximum of generation. For α-dynamo, the maximum is at the extremum of the α-effect. Fo
Publikováno v:
Geophysical & Astrophysical Fluid Dynamics. 52:125-139
We propose a method of derivation of global asymptotic solutions of the hydromagnetic dynamo problem at large magnetic Reynolds number. The procedure reduces to matching the local asymptotic forms for the magnetic field generated near individual extr