Zobrazeno 1 - 10
of 13
pro vyhledávání: '"L. L. KICHATINOV"'
Autor:
Valery V. Pipin, L. L. Kichatinov
Publikováno v:
Astronomy Reports. 44:771-779
the effect of the large-scale magnetic fields generated by the solar dynamo on the radiation flux issuing from the convection zone is studied. A governing equation describing convective heat transfer is obtained in the framework of mean-field magneto
Autor:
L. L. Kichatinov
Publikováno v:
Solar Physics. 133:177-194
An axisymmetric model for the Sun's differential rotation based upon a mechanism for angular momentum transport by compressible convection is developed. Convective heat transport is also considered. The model is simplified by the neglect of meridiona
Autor:
V. N. Krivodubskij, L. L. Kichatinov
Publikováno v:
The Sun and Cool Stars: activity, magnetism, dynamos ISBN: 9783540539551
The influence of rotation on the transfer of the mean magnetic field of the Sun, caused by the radial inhomogeneity of the solar turbulent plasma density, is investigated. It turns out that the transfer directions of the poloidal and toroidal magneti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::19158902d0e7ec74a633abc5b1929a5b
https://doi.org/10.1007/3-540-53955-7_127
https://doi.org/10.1007/3-540-53955-7_127
Autor:
L. L. Kichatinov
Publikováno v:
Geophysical & Astrophysical Fluid Dynamics. 54:145-160
Fluxes of angular momentum produced by turbulence in rotating fluids are derived with the effects of a magnetic field included. It is assumed that the rotation is slow but that the magnetic field is of arbitrary strength. A mean magnetic field is sho
Autor:
L. L. Kichatinov
Publikováno v:
The Cosmic Dynamo ISBN: 9780792325475
The effect of anisotropic transport of the mean magnetic field by turbulence in a stratified rotating fluid is briefly discussed to find its qualitative correspondence to the observed field redistribution over a solar cycle. A kinematic model of a dy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d8ce27f26e869ded1a60d9c6aed0a5f3
https://doi.org/10.1007/978-94-011-0772-3_2
https://doi.org/10.1007/978-94-011-0772-3_2
Autor:
L. L. Kichatinov
Publikováno v:
Solar Photosphere: Structure, Convection, and Magnetic Fields ISBN: 9780792305309
The present status of the Sun’s differential rotation theories is reviewed. Attention is mainly focused on mechanisms for differential rotation based on the anisotropic viscosity concept and their modern developments within the framework of the mea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3527164547fe2b920e3c9da9f60fb9cd
https://doi.org/10.1007/978-94-009-1061-4_32
https://doi.org/10.1007/978-94-009-1061-4_32
Autor:
L. L. Kichatinov
Publikováno v:
Geophysical & Astrophysical Fluid Dynamics. 35:93-110
With the help of simplifying approximations, we have derived expressions for the non-diffusive fluxes of the angular momentum which are brought about by the action of Coriolis forces on the convective motion. The original turbulence, which is not per
Autor:
L. L. Kichatinov
Publikováno v:
Radiophysics and Quantum Electronics. 26:427-431
Autor:
L. L. Kichatinov
Publikováno v:
Astronomische Nachrichten: A Journal on all Fields of Astronomy. 309:197-211
The mean electromotive force and the turbulent stress tensor are derived for an inhomogeneously turbulent conducting fluid under global rotation. The influence of the mean magnetic field on microscale turbulence is taken into account. As a result, th