This paper reports a large southward magnetic field of -23.5 nT in the
Earth's magnetotail at a radial distance of 46 R-E, observed with Geo
tail on January 10, 1995. The large southward field was part of a bipo
lar B-z signature of a plasmoid in association with a well-isolated su
bstorm under steady solar wind conditions. Magnetic field and plasma o
bservations are analyzed and compared with results from a hybrid simul
ation for magnetic reconnection, The large southward field is produced
by the piling up of field lines due to colliding fast tailward flowin
g plasmas. This study implies that the piling-up mechanism plays an im
portant role in the evolution of plasmoids traveling in the magnetotai
l.