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Bursty bulk flows in the inner central plasma sheet

Journal Article · · Journal of Geophysical Research; (United States)
DOI:https://doi.org/10.1029/91JA02701· OSTI ID:5556440
; ; ; ; ;  [1]; ;  [2];  [3]
  1. Univ. of California, Los Angeles (United States)
  2. Max-Planck-Inst. fuer extraterrestrische Physik, Garching (West Germany)
  3. Univ. Braunschweig (West Germany)
High speed flow in the inner central plasma sheet are studied, together with the concurrent behavior of the plasma and magnetic field, by using AMPTE/IRM data from {approx} 9 to 19 R{sub E} in the Earth's magnetotail. The conclusions drawn from the detailed analysis of a representative event are reinforced by a superposed epoch analysis on 2 years of data. The high-speed flows organize themselves in 10-min time scale flow enhancements which they call bursty bulk flow (BBF) events. Both temporal and spatial effects are responsible for their bursty nature. The flow velocity exhibits peaks of very large amplitude with a characteristic time scale of the order of a minute, which are usually associated with magnetic field dipolarizations and ion temperatures increases. The BBFs represent intervals of enhanced earthward convection and energy transport per unit area in the y-z GSM direction of the order of 5 {times} 10{sup 19} ergs/R{sub E}{sup 2}.
OSTI ID:
5556440
Journal Information:
Journal of Geophysical Research; (United States), Journal Name: Journal of Geophysical Research; (United States) Vol. 97:A4; ISSN JGREA; ISSN 0148-0227
Country of Publication:
United States
Language:
English

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