Rotating Convection in an Anisotropic System
with Alex Roxin
Phys. Rev. E 65 (2002) 046219
We study the stability of patterns arising in rotating
convection in weakly anisotropic systems using a modified
Swift-Hohenberg equation. The anisotropy, either an endogenous
characteristic of the system or induced by external forcing,
can stabilize periodic rolls in the Küppers-Lortz chaotic
regime. For the particular case of rotating convection with
time-modulated rotation where recently, in experiment, chiral
patterns have been observed in otherwise Küppers-Lortz-unstable
regimes, we show how the underlying base-flow breaks the
isotropy, thereby affecting the linear growth-rate of
convection rolls in such a way as to stabilize spirals and
targets. Throughout we compare analytical results to numerical
simulations of the Swift-Hohenberg equation.
movie (300kB) of spiral with irregular pattern evolution in core.
Last modified: February 9, 2003
Hermann Riecke (h-riecke at northwestern.edu)
|