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Statistical characteristics of plasma flow in the magnetotail

Journal Article · · J. Geophys. Res.; (United States)
The characteristics of plasma flow are studied statistically by using the IMP 6 plasma and magnetic field data. The analysis was performed by dividing the data set according to flow direction and flow velocity. Fast tailward flows (those with a tailward component of velocity exceeding 300 km/s) are observed only within a few R/sub E/ of the estimated neutral sheet position and are associated with southward polarity of the magnetic field. They can therefore be interpreted as a product of reconnection operating at a location earthward of the spacecraft. On the other hand, slow tailward flows (those with a tailward component less than 300 km/s) are not associated with southward field polarity and are very similar to slow earthward flow (those with an anti-tailward component less than 300 km/s) in such characteristics as association to northward inclination of the field and occurrence over a wide range of distance ( +- several R/sub E/) from the neutral sheet. These results suggest that there exist at least two source mechanisms of plasma flow in the magnetotail; X type neutral line in the near-earth plasma sheet is likely to be the source of the fast tailward flows but other driving mechanism are responsible for slow flows.
Research Organization:
The Institute of Space and Astronautical Science, Komaba, Meguro-ku, Tokyo 153, Japan
OSTI ID:
5199921
Journal Information:
J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 87:A1; ISSN JGREA
Country of Publication:
United States
Language:
English

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