The linear dynamics of the unstably stratified geophysical flows is in
vestigated with a two-layer formulation. A 'convective' deformation ra
dius classifies the dynamics into three regimes: 1. the scales smaller
than the deformation radius: the dynamics characterized by unstable i
nertial-gravity modes; 2, the scales larger than the deformation radiu
s: a quasi-geostrophic regime; 3, the scales close to the deformation
radius, where the dynamics transits from the inertial-gravity regime t
o the quasi-geostrophic regime. The Rossby wave can propagate eastward
in the unstably stratified quasi-geostrophic regime, The baroclinic i
nstabilities are basically realized as a larger-scale extent of the in
ertial-gravity instabilities, but the former can be isolated from the
latter in a limit of small p-effect, with a very deep lower layer. The
results suggest that the convectively unstable Jovian atmospheric dyn
amics can be well described as a quasi-geostrophic system.