In this paper, we describe a global synthesis dipolarization model combinin
g coupled processes in the midtail, inner tail and auroral ionosphere: In t
he late growth phase, magnetic reconnection releases the magnetic energy st
ored in the magnetotail. Magnetic flux and energy are transported earthward
and tailward. As earthward flow slows down in the near-earth plasma sheet
(NEPS), it compresses the magnetic field acid plasmas near and earthward of
the inner edge of the NEPS and pushes them further inward (earthward and e
quatorward). This sets up a favorable condition for generating the drift ba
llooning mode (DBM) instability in the inner tail. The unstable DBMs genera
te coupled Alfven-slow magnetosonic waves and field-aligned currents (FACs)
, resulting in a turbulent state in the equatorial region and enhancing the
ionospheric conductance Sigma. As soon as Sigma and FACs increase to a thr
eshold level, the substorm current wedge is formed, leading to an explosive
intensification of the auroral electrojet and magnetic field dipolarizatio
n at substorm onset. Moreover, we regard the "substorm trigger phase" (Ohta
ni et al., Planet. Space Sci. 37 (1989) 579-588) as the interval during whi
ch the inner tail is being further compressed inward and the DBMs explosive
ly develop to trigger magnetic field dipolarization. We suggest that the da
wn-dusk electric field E-y which causes further compression of the inner ta
il may either be associated with flow braking, or produced by storm SSC and
other magnetospheric processes. The present model is thus applicable to th
e cases either with or without neutral-line formation. Furthermore, in the
former case, the enhanced E-y in the inner tail may either appear somewhat
later than or simultaneously with magnetic reconnection in the midtail. It
seems that a variety of expansion onset features can be explained in terms
of this synthesis dipolarization model. (C) 2001 Elsevier Science Ltd. All
rights reserved.