Study of the Preferential Acceleration and Merging of Coherent Structures, BBF and Intermittent Turbulence in Earth's Magnetotail

Physics

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2700 Magnetospheric Physics, 2708 Current Systems (2409), 2744 Magnetotail, 2753 Numerical Modeling, 2788 Storms And Substorms

Scientific paper

Recent satellite observations indicate that the Earth's magnetotail is generally in a state of intermittent turbulence constantly intermixed with localized busty bulk flows (BBF) [Angelopoulos et al., J. Geophys. Res., 97, 4027, 1992; Lui et al., Geophys. Res. Lett., 15, 721, 1988]. A model of sporadic and localized merging of coherent structures has been proposed by Chang [Phys. Plasmas, 6, 4137, 1999] to describe the dynamics of the magnetotail. When conditions are favorable, the coherent structures may merge, interact, convect and evolve into forced and/or self-organized critical (FSOC) states [Chang, IEEE Trans. Plasma Sci., 20, 691, 1992], a condition satisfied by the observational statistics of the characteristics of the BBF [Angelopoulos, Phys. Plasmas, 6, 4161, 1999]. When considered with the realistic magnetotail geometry, the coarse-grained dissipation of turbulent fluctuations produced by the interacting multi-scale coherent structures may induce global nonlinear instabilities and possibly trigger substorms. Some of the above ideas have been demonstrated by direct numerical simulaions [Wu and Chang, Geophys. Res. Lett., 27, 863, 2000]. In this paper, we address the dynamics, particularly the preferential acceleration, of the coherent structures in a sheared magnetic field geometry. Preliminary comparisons of the theoretical ideas and new numerical results with the observed characteristics of BBF will also be presented.

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