Hi. Lu et Tl. Miller, CHARACTERISTICS OF ANNULUS BAROCLINIC FLOW STRUCTURE DURING AMPLITUDEVACILLATION, Dynamics of atmospheres and oceans, 27(1-4), 1998, pp. 485-503
An investigation is made of the mechanics of amplitude vacillation in
a numerically simulated rotating annulus flow system. Amplitude vacill
ation is characterized by a periodic change of vertical wave structure
in concert with growth and decay of wave amplitude and phase speed. T
he temperature wave amplitude profile for the dominant component consi
sts of three local maxima: (1) lower boundary layer, (2) upper half la
yer and (3) lower half layer. The lower layer waves lead the time-depe
ndent structural variation during vacillation. Two types of amplitude
vacillation found in the experimental measurements (Buzyna et al., 198
9: J. Atmos. Sci. 46, 2716-2729) can be distinguished in the temperatu
re wave by whether the lower layer waves split from and travel behind
the upper layer waves by one wave period in each cycle of vacillation.
Linear eigenvalue analyses with respect to the instantaneous axisymme
tric state at various points in time are performed to elucidate the si
mple interaction between the dominant wave and the zonal mean state, D
uring the vacillation cycle, the zonal mean state is modified by the w
ave, which causes a change in growth rate and vertical structure of th
e linearly most unstable eigenmode. This, in turn, forces the actual c
hanges of the nonlinear solutions. (C) 1997 Elsevier Science B.V.