The field-aligned current densities in the core of a magnetotail flux
rope were directly detected with plasma instrumentation on board the G
eotail spacecraft at a downstream distance of about 96 R(E) (Earth rad
ii). The axis of the flux rope and the core magnetic fields were direc
ted cross-tail, and the magnitudes of these core magnetic fields were
similar to that in the magnetotail lobe at these distances. The radius
of the core cross-section was about 0.7 R(E), and the total current w
as 500,000 A. Together with a recently reported, similar measurement w
ith the Galileo spacecraft these direct detections of current greatly
strengthen the previous identifications in favor of flux ropes that we
re solely based on their magnetic signatures. The detection of the flu
x rope with the Geotail spacecraft occurred during a period of relativ
e magnetic quiescence.