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  2. Kelvin–Helmholtz instability - Wikipedia

    en.wikipedia.org/wiki/KelvinHelmholtz_instability

    A KH instability rendered visible by clouds, known as fluctus, [2] over Mount Duval in Australia A KH instability on the planet Saturn, formed at the interaction of two bands of the planet's atmosphere Kelvin-Helmholtz billows 500m deep in the Atlantic Ocean Animation of the KH instability, using a second order 2D finite volume scheme

  3. What are Kelvin-Helmholtz clouds? Rare formation spotted over ...

    www.aol.com/news/kelvin-helmholtz-clouds-rare...

    A curious cloud seen over Smith Mountain looks more like something out of a fairytale than it does real life — and the science behind it is fascinating. What are Kelvin-Helmholtz clouds?

  4. 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 KelvinHelmholtz instability forming in clouds. The KelvinHelmholtz 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.

  5. Mammatus cloud - Wikipedia

    en.wikipedia.org/wiki/Mammatus_cloud

    KelvinHelmholtz (K–H) instability is prevalent along cloud boundaries and results in the formation of wave-like protrusions (called Kelvin-Helmholtz billows) from a cloud boundary. Mammatus are not in the form of K-H billows, thus, it is proposed that the instability can trigger the formation of the protrusions, but that another process ...

  6. Jeans instability - Wikipedia

    en.wikipedia.org/wiki/Jeans_instability

    Jeans instability; KelvinHelmholtz mechanism; ... The Jeans instability is a concept in astrophysics that describes an instability that ... The cloud is stable for ...

  7. Kelvin–Helmholtz mechanism - Wikipedia

    en.wikipedia.org/wiki/KelvinHelmholtz_mechanism

    The KelvinHelmholtz mechanism is an astronomical process that occurs when the surface of a star or a planet cools. The cooling causes the internal pressure to drop, and the star or planet shrinks as a result. This compression, in turn, heats the core of the star/planet.

  8. List of cloud types - Wikipedia

    en.wikipedia.org/wiki/List_of_cloud_types

    Lens-shaped middle cloud. Includes informal variant altocumulus KelvinHelmholtz cloud, lenticular spiral indicative of severe turbulence. Altocumulus volutus (V-27) Elongated, tube shaped, horizontal stratocumuliform cloud. Altocumulus castellanus (V-28) Turreted layer cloud. Altocumulus floccus (V-29) Tufted stratocumuliform clouds with ...

  9. Kelvin Harrison Jr. Reveals How He Developed His Own ... - AOL

    www.aol.com/entertainment/kelvin-harrison-jr...

    Kelvin Harrison Jr. is ready to show fans a whole new version of the iconic Disney villain Scar. The actor, 30, exclusively told Us Weekly that he initially approached his role in Mufasa: The Lion ...