The model of turbulent plasma sheet during IMF Bz > 0

Details The model of turbulent plasma sheet during IMF Bz > 0 The model of turbulent plasma sheet during IMF Bz > 0

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001adspr..28.1747a&link_type=abstract

Advances in Space Research, Volume 28, Issue 12, p. 1747-1752.

Physics

5

Scientific paper

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.

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