One of the striking features of tropical instability waves (TIWs) is t
hat they appear to be more prominent north of the equator. A linearize
d, 2 1/2-layer ocean model is used to investigate effects of various a
symmetric background states on structures of equatorial, unstable wave
s. Our results suggest that the meridional asymmetry of TIWs is due to
asymmetries of the two branches of the South Equatorial Current (SEC)
and of the equatorial, sea surface temperature front; it is not due t
o the presence of the North Equatorial Countercurrent. Energetics anal
yses indicate that frontal instability associated with the equatorial,
SST front, as well as barotropic instability due to shear associated
with the SEC, are energy sources for the model TIWs.