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Observations indicate that the magnetotail convection is turbulent andbi-modal, consisting of fast bursty bulk flows (BBF) and a nearly stagnantbackground. We demonstrate that this observed phenomenon may be understood interms of the intermittent interactions, dynamic mergings and preferentialaccelerations of coherent magnetic structures under the influence of abackground magnetic field geometry that is consistent with the development ofan X-point mean-field structure.Comment: 12 pages, 5 Postscript figures, uses agums.st

Preferential Acceleration of Coherent Magnetic Structures and Bursty Bulk Flows in Earth's Magnetotail