Physics – Space Physics
Scientific paper
2001-06-28
Physics
Space Physics
12 pages, 5 Postscript figures, uses agums.sty
Scientific paper
10.1238/Physica.Topical.098a0004
Observations indicate that the magnetotail convection is turbulent and bi-modal, consisting of fast bursty bulk flows (BBF) and a nearly stagnant background. We demonstrate that this observed phenomenon may be understood in terms of the intermittent interactions, dynamic mergings and preferential accelerations of coherent magnetic structures under the influence of a background magnetic field geometry that is consistent with the development of an X-point mean-field structure.
Angelopoulos Vassilis
Chang Tom
Wu Cheng-chin
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