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  2. Kelvin–Helmholtz instability - Wikipedia

    en.wikipedia.org/wiki/Kelvin–Helmholtz_instability

    The study of this instability is applicable in plasma physics, for example in inertial confinement fusion and the plasma–beryllium interface. In situations where there is a state of static stability (where there is a continuous density gradient), the Rayleigh-Taylor instability is often insignificant compared to the magnitude of the Kelvin ...

  3. Two-stream instability - Wikipedia

    en.wikipedia.org/wiki/Two-stream_instability

    The two-stream instability is a very common instability in plasma physics. It can be induced by an energetic particle stream injected in a plasma, or setting a current along the plasma so different species (ions and electrons) can have different drift velocities. The energy from the particles can lead to plasma wave excitation. [1]

  4. Instability - Wikipedia

    en.wikipedia.org/wiki/Instability

    Hydrodynamics simulation of the Rayleigh–Taylor instability [3] Unstable flow structure generated from the collision of two impinging jets.. Fluid instabilities occur in liquids, gases and plasmas, and are often characterized by the shape that form; they are studied in fluid dynamics and magnetohydrodynamics.

  5. Hydrodynamic stability - Wikipedia

    en.wikipedia.org/wiki/Hydrodynamic_stability

    This is an image, captured in San Francisco, which shows the "ocean wave" like pattern associated with the Kelvin–Helmholtz instability forming in clouds. The Kelvin–Helmholtz instability (KHI) is an application of hydrodynamic stability that can be seen in nature. It occurs when there are two fluids flowing at different velocities.

  6. Modulational instability - Wikipedia

    en.wikipedia.org/wiki/Modulational_instability

    In the fields of nonlinear optics and fluid dynamics, modulational instability or sideband instability is a phenomenon whereby deviations from a periodic waveform are reinforced by nonlinearity, leading to the generation of spectral-sidebands and the eventual breakup of the waveform into a train of pulses. [1] [2] [3]

  7. Rayleigh–Taylor instability - Wikipedia

    en.wikipedia.org/wiki/Rayleigh–Taylor_instability

    This figure represents the evolution of the Rayleigh–Taylor instability from small wavelength perturbations at the interface (a) which grow into the ubiquitous mushroom shaped spikes (fluid structures of heavy into light fluid) and bubbles (fluid structures of light into heavy fluid) (b) and these fluid structures interact due to bubble merging and competition (c) eventually developing into ...

  8. College Football Playoff: Who has the best odds to win the title?

    www.aol.com/college-football-playoff-best-odds...

    The first 12-team College Football Playoff field was revealed on Sunday. Undefeated Oregon earned the top seed, while SMU beat out Alabama for the 12th and final spot. Oregon, Georgia, Boise State ...

  9. Plasma stability - Wikipedia

    en.wikipedia.org/wiki/Plasma_stability

    Helical kink instability (a.k.a. helical instability) Rayleigh–Taylor instability (RTI, a.k.a. gravitational instability) Rotating instability, [30] Tearing mode instability (or resistive tearing instability [31]) Two-stream instability (a.k.a. beam-plasma instability, counter-streaming instability) Beam acoustic instability; Bump-on-tail ...

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