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Showing 1 to 9 of 9 for “"Fluid instabilities"”.

  1. Instabilities and flow-induced structures in anisotropic systems

    … is driven out of equilibrium. Nature leverages instabilities to ‘fabricate’ complex structures that maximize performance using minimal resources, exploiting the self-amplification of small perturbations. The potential to use instabilities in practical applications, for example to engineer or …

    mit Repository record for Instabilities and flow-induced structures in anisotropic systems (opens in a new tab)

  2. Oblique shock interactions with gas cylinder interfaces

    This thesis presents an experimental study of fluid instabilities formed due to an oblique interatction of a shock wave with a cylindrical gas column seeded with glycol droplets. Two gases are injected into quiescent air to form the column. The first is sulfur hexafluoride (SF6) which generates the …

    unm Repository record for Oblique shock interactions with gas cylinder interfaces (opens in a new tab)

  3. Midlatitude sporadic-E layers

    … cases to critical level effects and in others to fluid instabilities. The convergence of a meteor trail can, under some circumstances, account for localized enhancement of the electron density in the layer.

    uiuc Repository record for Midlatitude sporadic-E layers (opens in a new tab)

  4. Multifluid Kelvin-Helmholtz instability in weakly ionised astrophysical plasmas

    … ionised astrophysical plasma flows in a multifluid regime. This numerical study is carried out using the multifluid MHD code HYDRA. An outline of the structure of this code is given in chapter 2 and the schemes which are implemented integrates the MHD equations. We are interested in multifluid …

    dcu Repository record for Multifluid Kelvin-Helmholtz instability in weakly ionised astrophysical plasmas (opens in a new tab)

  5. Oblique shock interactions With perturbed density interfaces

    … an experimental and numerical consideration of fluid instabilities formed by the interaction of a planar shock wave and a cylindrical column of gas seeded with glycol droplets. Seeding a fluid flow with a passive tracer is a common practice in experimental fluids research and it is important to …

    unm Repository record for Oblique shock interactions With perturbed density interfaces (opens in a new tab)

  6. The impact and rupture of a water-filled balloon on a rigid surface

    The dropping of a water-filled latex balloon onto a flat, rigid surface is an experiment that is known and has been performed by many, but on which there is no existing published work. High-speed images taken of the process revealed a range of phenomena, many of which had not been previously …

    cambridge Repository record for The impact and rupture of a water-filled balloon on a rigid surface (opens in a new tab)

  7. Influence of external environment on fluid/ion transport in confined nanoscale systems

    … micro-nano junction owing to the convective fluid instabilities. Experimental works were navigated this field of research and postulated a probable convective fluid and charge instabilities for the overlimiting current characteristics in micro-nanostructures. However, an exact physical …

    uiuc Repository record for Influence of external environment on fluid/ion transport in confined nanoscale systems (opens in a new tab)

  8. Planet formation, resonant drag instabilities, and vortices

    … the mechanism I uncover drives a whole class of instabilities called ‘resonant drag instabilities’ (RDIs). These appear in mixtures of gas and dust, when the two species drift relative to each other. I use linear perturbation theory and asymptotic methods in the limit of dilute dust to show that …

    cambridge Repository record for Planet formation, resonant drag instabilities, and vortices (opens in a new tab)

  9. Star formation and disk stability in nearby galaxies

    … models. (i) The thin gas-disk model (single-fluid disk criterion, Qg) was derived for each galaxy in our sample. We use atomic gas for the majority of the sample and we use molecular gas whenever available. (ii) A two-fluid disk criterion which models a galaxy disk with gas and stars as two …

    cape-town Repository record for Star formation and disk stability in nearby galaxies (opens in a new tab)