Conveners
Wednesday Afternoon
- Philip Armitage (University of Colorado)
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22. Linear stability of accretion disks under the influence of stratification and thermal relaxationDr Hubert Klahr (MPIA)06/08/2014, 14:00Workshop Main ProgrammeKeplerian disks have proven to be extremely stable to perturbations, when magnetic fields are not in operation. But disks around young stars are complicated entities - they share a lot of properties with planetary atmospheres and one can learn a lot from the stability of rotating stars. Disks around young stars have a radial temperature gradient driven by stellar irradiation, which leads to a...Go to contribution page
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Prof. Richard Nelson (Queen Mary University of London)06/08/2014, 14:30Workshop Main ProgrammeAccretion discs with radial temperature gradients have angular velocity profiles that vary both with radius and height. The presence of vertical shear can lead to a hydrodynamic instability (the vertical shear instability - VSI) that is essentially a manifestation of the Goldreich-Schubert-Fricke instability in the disc context. In this talk I will present the results from a recent study in...Go to contribution page
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Dr Martin Pessah (Niels Bohr International Academy)06/08/2014, 15:30Workshop Main ProgrammeThe shearing box has been extensively used for studying local processes in accretion disks. This framework is appropriate for studying barotropic disks, for which the pressure is only a function of the density and the angular frequency is independent of height. I will introduce a more general framework by showing that, given a global disk model, it is possible to develop consistent models that...Go to contribution page
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06/08/2014, 16:00