Geotail observed a fast tailward flow burst (a speed of >600 km/s) wit
h southward B-z in the Earth's magnetotail at a radial distance of 15.
5 R-E on March 30, 1995. Ions in this burst consisted of a single-comp
onent plasma showing convection motion, and these ions were confined n
ear the neutral sheet. This flow burst was likely associated with a ps
eudobreakup rather than a major substorm onset. In this event, magneti
c reconnection appeared to take place only for the field lines near th
e neutral sheet. The magnetic reconnection was quenched soon and resul
ted in a short-lived tailward flow burst embedded in the plasma sheet.