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Natural convection is usually complicated by additional factors such asrotation, shear, radiative transfer, compressibility and electromagnetic fields(in the case of electro-conductive fluids). It is shown, using results ofnumerical simulations and measurements in atmospheric boundary layer and solarphotosphere that strong stratification can transform turbulence intodeterministic chaos with exponential spectral decay of kinetic energy. When thestratification becomes weaker the deterministic chaos is replaced by thedistributed chaos with stretched exponential spectral decay controlled by thesecond or third moments of the helicity distribution.

Stratification versus turbulence in complex convection