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Outline: • Capturing Dust in Pressure maxima e.g. Zonal flows and vortices • MHD turbulence and Gravoturbulent Planetesimal formation -> Karsten Dittrich • Turbulence and vortices in Baroclinic disks: Disk Weather • Modified Symmetric Instability • Dust capturing in 3D vortices • Summary, Conclusions 12/13/2009 Hubert Klahr - Planet Formation - MPIA Heidelberg Wednesday, September 5, 12 The role of Turbulence in Planet Formation
Turbulence in a non rotating frame: Cuzzi et al. 12/13/2009 Hubert Klahr - Planet Formation - MPIA Heidelberg Wednesday, September 5, 12 L H Laboratory Conditions Dust collects between vortices (high pressure)
Page 1: The Role of Turbulence in Planetesi
Page 5 and 6: V e r t i c a l From dust/gas eq. 1
Page 7 and 8: Disk: 12/13/2009 Hubert Klahr - Pla
Page 9 and 10: Formation Of Planetesimals From pre
Page 11 and 12: Not the process but numerical resol
Page 13 and 14: Natalia Dziurkevich (in prep.) see
Page 15 and 16: 12/13/2009 Hubert Klahr - Planet Fo
Page 17 and 18: Ri 0.001 0.000 �0.001 �0.002
Page 19 and 20: 12/13/2009 Hubert Klahr - Planet Fo
Page 21 and 22: 2D axissymetric Pluto Simulation: T
Page 23 and 24: 2D axissymetric Pluto Simulation: R
Page 25 and 26: Interface MRI - Dead Zone linear ax
Page 27 and 28: Small particles in pressure maxima
Page 29 and 30: St = 0.05 particles (few millimeter
Page 31: Conclusions: Johansen and Klahr: Hi

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