TY - GEN A1 - Helling, Christiane A1 - Klein, Rupert A1 - Woitke, Peter A1 - Nowak, Ulrich A1 - Sedlmayr, Erwin T1 - Dust in Brown Dwarfs IV. Dust formation and driven turbulence on mesoscopic scales N2 - Dust formation {in brown dwarf atmospheres} is studied by utilizing a model for driven turbulence in the mesoscopic scale regime. We apply a pseudo-spectral method where waves are created and superimposed {within} a {limited} wavenumber interval. The turbulent kinetic energy distribution follows the Kolmogoroff spectrum which is assumed to be the most likely value. Such superimposed, stochastic waves may occur in a convectively active environment. They cause nucleation fronts and nucleation events and thereby initiate the dust formation process which { continues until} all condensible material is consumed. Small disturbances {are found to} have a large impact on the dust forming system. An initially dust-hostile region, which may originally be optically thin, becomes optically thick in a patchy way showing considerable variations in the dust properties during the formation process. The dust appears in lanes and curls as a result of the interaction with waves, i.e. turbulence, which form larger and larger structures with time. Aiming on a physical understanding of the variability of brown dwarfs, related to structure formation in substellar atmospheres, we work out first necessary criteria for small-scale closure models to be applied in macroscopic simulations of dust forming astrophysical systems. T3 - ZIB-Report - 03-33 KW - substellar atmospheres KW - dust formation KW - turbulence Y1 - 2003 UR - https://opus4.kobv.de/opus4-zib/frontdoor/index/index/docId/755 UR - https://nbn-resolving.org/urn:nbn:de:0297-zib-7555 ER -