We focus on the influence of the beta -effect on the singular modes of baro
clinic instability in the Phillips model. An analytical intercomparison bet
ween normal and singular modes for the Eady problem on an f-plane has alrea
dy been performed, showing that the amplification rate of the singular mode
for the kinetic-energy norm after a dimensional time of three days is abou
t 1.2 times larger than for the normal mode. We show here that, in the pres
ence of the beta -effect, the maximum amplification rate of the singular mo
de can be 1.5 times larger than for the normal-mode case. This difference i
s due to the lesser stabilizing effect of beta on the singular modes compar
ed with the normal modes. This result is obtained for the case of equal lay
er depths which is relevant for the atmospheric situation. For the oceanic
situation with unequal layer depths the amplification due to beta is furthe
r increased leading to a factor of 1.8 in amplification rates between the t
wo types of modes after a dimensional time of about 20 days. This behaviour
is explained by the fact that beta only intervenes in the anti-Hermitian p
art of the linear dynamical operator, the main effect of which is to alter
the vertical phase tilt of the perturbations. As a consequence, the structu
re of the bi-orthogonal mode becomes more inclined to the vertical in the p
resence of beta while, on the contrary, the structure of the unstable norma
l mode becomes less inclined.