Next: Far-Field
Breakup Up: Spiral
Wave Spectra Previous: Meander
Reaction-diffusion
equations with M. Bär and M. Eiswirth kinetics [8]
are simulated. The initial condition is a stable rotating spiral for
.
At the beginning of the simulation
is changed to
.
The spiral wave breaks up close to the core (center) of the spiral.
Linear stability computations as these parameter values show that the
spiral is linearly unstable.
Model Parameters for simulation:
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