The model of turbulent plasma sheet during IMF Bz > 0
Abstract
Theory of the plasma sheet with medium-scale developed turbulence gives the possibility to explain the main processes of plasma sheet bifurcation and theta-aurora formation during IMF Bz > 0. The model suggests that during IMF Bz > 0 small bulge structure in the plasma sheet center is formed. The polarization of the bulge due to dawnward electron motion and duskward ion motion decreases the large-scale electric field in the bulge region. The decrease of the large-scale field in the conditions of constant coefficient of diffusion leads to the bulge growth. The results of plasma sheet bifurcation and theta-aurora formation modelling are presented.
Más información
Título de la Revista: | ADVANCES IN SPACE RESEARCH |
Volumen: | 28 |
Número: | 12 |
Editorial: | ELSEVIER SCI LTD |
Fecha de publicación: | 2001 |
Página de inicio: | 1747 |
Página final: | 1752 |
URL: | http://linkinghub.elsevier.com/retrieve/pii/S0273117701005415 |
DOI: |
10.1016/S0273-1177(01)00541-5 |
Notas: | ISI, SCOPUS |