GEOTAIL SURVEY OF ION FLOW IN THE PLASMA SHEET - OBSERVATIONS BETWEEN10 AND 50 R-E

Citation
Wr. Paterson et al., GEOTAIL SURVEY OF ION FLOW IN THE PLASMA SHEET - OBSERVATIONS BETWEEN10 AND 50 R-E, J GEO R-S P, 103(A6), 1998, pp. 11811-11825
Citations number
30
Categorie Soggetti
Geosciences, Interdisciplinary","Astronomy & Astrophysics","Metereology & Atmospheric Sciences",Oceanografhy,"Geochemitry & Geophysics
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN journal
21699380 → ACNP
Volume
103
Issue
A6
Year of publication
1998
Pages
11811 - 11825
Database
ISI
SICI code
2169-9380(1998)103:A6<11811:GSOIFI>2.0.ZU;2-F
Abstract
One-minute samples of the velocity distributions of ions are used to c ompute plasma moments for the 18-month period between December 1, 1994 and Tune 1, 1996. Statistical analyses of these measurements are give n for the plasma sheet and its boundary layer at radial distances from Earth between 10 and 50 R-E Analysis concentrates on examination of p arallel and perpendicular components of bulk flow and is directed towa rd understanding processes that affect transport. On average, the perp endicular components of the bulk flow are small, less than 15 km/s. On the basis of this study, two distinct patterns emerge. First, at radi al distances from Earth less than 30 R-E the mean perpendicular flow i ndicates a well-defined pattern of convection that is a combination of drift toward Earth and drift toward the flanks. The average electric field across the tail is inferred to be 0.1 mV/m. Second, there is a n otable increase in the variability of the perpendicular flow speeds be yond 25 R-E Al relatively large bulk flows with speeds in the range 20 0 to 800 km/s are sometimes found in the tail at lesser radial distanc e, these are primarily field-aligned and thus do not contribute substa ntially to convection or to the transport of magnetic flux.