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Showing 1 to 5 of 5 for “"inertial modes"”.

  1. Tidal Dissipation in Extrasolar Planets

    … explain the observed Q value. The only normal modes that fall in the frequency range of the tidal forcing (~ few days) are inertial modes, modes restored by the Coriolis force. We present a new numerical technique to solve for inertial modes in a convective, rotating sphere. This technique …

    toronto-retro Repository record for Tidal Dissipation in Extrasolar Planets (opens in a new tab)

  2. Rotating, hydromagnetic laboratory experiment modelling planetary cores

    … fluid. We have observed and identified inertial modes, which are bulk oscillations of the fluid restored by the Coriolis force. Over-reflection at a shear layer is one mechanism capable of exciting such modes, and we have developed predictions of both onset boundaries and mode selection …

    maryland Repository record for Rotating, hydromagnetic laboratory experiment modelling planetary cores (opens in a new tab)

  3. Shearing waves and the MRI dynamo in stratified accretion discs

    … first, generation of acoustic waves by mixing of inertial waves, and second, the generation of a self-sustaining magnetic field via the magnetorotational instability (MRI) which would be a source of dissipative turbulence. Previous local simulations of the MRI have shown that the dynamo changes …

    cambridge Repository record for Shearing waves and the MRI dynamo in stratified accretion discs (opens in a new tab)

  4. Variability of black-hole accretion discs: a theoretical study

    … to viscous overstability. The overstable inertial-acoustic waves appear to be excited near the maximum of the epicyclic frequency and are global in the sense that their frequency is maintained for a wide range of radii. The second class of models looks at accretion-disc oscillations which …

    cambridge Repository record for Variability of black-hole accretion discs: a theoretical study (opens in a new tab)