Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Kh. Z. Chargazia"'
Publikováno v:
Nonlinear Processes in Geophysics, Vol 16, Iss 1, Pp 11-22 (2009)
This paper investigates the macroscopic consequences of nonlinear solitary vortex structures in magnetized space plasmas by developing theoretical model of plasma turbulence. Strongly localized vortex patterns contain trapped particles and, propagati
Externí odkaz:
https://doaj.org/article/b6184a15a0c64f4c891585309e5a18ad
Autor:
Kh. Z. Chargazia, Oleg Kharshiladze
Publikováno v:
Geomagnetism and Aeronomy. 57:207-216
A theoretical-numerical description of zonal flow generation in the turbulent ionosphere by controlled inhomogeneous background wind is given. The generalized Charney–Obukhov equation, which describes the nonlinear interaction of five different-sca
Publikováno v:
Geomagnetism and Aeronomy. 53:750-760
The generation and further nonlinear dynamics of internal gravity wave (IGW) structures in a dissipative ionosphere in the presence of an inhomogeneous zonal wind (shear flow) have been studied. The effectiveness of the IGW amplification mechanism du
Publikováno v:
Geomagnetism and Aeronomy. 53:650-654
A corresponding model system of nonlinear dynamic equations for the lower ionosphere has been constructed in order to study the generation and further nonlinear dynamics of internal gravity wave (IGW) structures in a dissipative ionosphere in the pre
Publikováno v:
Geomagnetism and Aeronomy. 53:362-366
The specific features of the generation and intensification of internal gravity wave structures in different atmospheric-ionospheric regions, caused by zonal local nonuniform winds (shear flows), are studied. The model of the medium has been explaine
Autor:
Kh. Z. Chargazia, G. D. Aburjania
Publikováno v:
Plasma Physics Reports. 37:177-190
A study is made of the generation and subsequent linear and nonlinear evolution of ultralow-frequency planetary electromagnetic waves in the E region of a dissipative ionosphere in the presence of a nonuniform zonal wind (a sheared flow). Hall curren
Autor:
Antonella Greco, Gaetano Zimbardo, Kh. Z. Chargazia, Luca Sorriso-Valvo, Zoltán Vörös, Olga Alexandrova, G. D. Aburjania, Silvia Perri
Publikováno v:
Space science reviews 156 (2010): 89.
info:cnr-pdr/source/autori:G. Zimbardo, A. Greco, L. Sorriso-Valvo, S. Perri, Z. Vörös, G. Aburjania, K. Chargazia, O. Alexandrova/titolo:Magnetic Turbulence in the Geospace Environment/doi:/rivista:Space science reviews/anno:2010/pagina_da:89/pagina_a:/intervallo_pagine:89/volume:156
Space Science Reviews
Space Science Reviews, 2010, 156, pp.89-134. ⟨10.1007/s11214-010-9692-5⟩
info:cnr-pdr/source/autori:G. Zimbardo, A. Greco, L. Sorriso-Valvo, S. Perri, Z. Vörös, G. Aburjania, K. Chargazia, O. Alexandrova/titolo:Magnetic Turbulence in the Geospace Environment/doi:/rivista:Space science reviews/anno:2010/pagina_da:89/pagina_a:/intervallo_pagine:89/volume:156
Space Science Reviews
Space Science Reviews, 2010, 156, pp.89-134. ⟨10.1007/s11214-010-9692-5⟩
International audience; Magnetic turbulence is found in most space plasmas, including the Earth's magnetosphere, and the interaction region between the magnetosphere and the solar wind. Recent spacecraft observations of magnetic turbulence in the ion
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 72:971-981
The generation and further linear and nonlinear dynamics of planetary ultra-low-frequency (ULF) waves are investigated in the rotating dissipative ionosphere in the presence of inhomogeneous zonal wind (shear flow). Planetary ULF magnetized Rossby ty
Publikováno v:
Planetary and Space Science. 57:1474-1484
In the present work, the generation of large-scale zonal flows and magnetic field by short-scale collision-less electron skin depth order drift-Alfven turbulence in the ionosphere is investigated. The self-consistent system of two model nonlinear equ
Publikováno v:
Nonlinear Processes in Geophysics, Vol 16, Iss 1, Pp 11-22 (2009)
Scopus-Elsevier
Scopus-Elsevier
This paper investigates the macroscopic consequences of nonlinear solitary vortex structures in magnetized space plasmas by developing theoretical model of plasma turbulence. Strongly localized vortex patterns contain trapped particles and, propagati