“…These may include: (i) the temperature profiles for the convection dominated thermoconduction and turbulent convection [9] (as in the convective zone of the sun and stars), (ii) stability and average profiles of granular materials (e.g., the sand pile profiles) and granular flows [2,3], (iii) equilibrium and steady state profiles of plasma pressure and temperature in fusion devices [8,10], etc. Despite its importance, the problem of spatial structure and characteristics of the SO steady states has received minor attention [7,[11][12][13]. In this Letter, we propose a method which is equally applicable to any CA provided its rules are rather simple.…”