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Rayleigh Taylor Instability
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High Quality Content by WIKIPEDIA articles! The Rayleigh Taylor instability, or RT instability (after Lord Rayleigh and G. I. Taylor), is an instability of an interface between two fluids of different densities, which occurs when the lighter fluid is pushing the heavier fluid. This is the case with an interstellar cloud and shock system. The equivalent situation occurs when gravity is acting on two fluids of different density with the dense fluid above a fluid of lesser density such as water balancing on light oil. Consider two completely plane-parallel layers of immiscible fluid, the heavier on top of the light one and both subject to the Earth's gravity. The equilibrium here is unstable to certain perturbations or disturbances. An unstable disturbance will grow and lead to a release of potential energy, as the heavier material moves down under the (effective) gravitational field, and the lighter material is displaced upwards. This was the set-up as studied by Lord Rayleigh.
Weitere Informationen
- Allgemeine Informationen
- GTIN 09786131104077
- Editor Lambert M. Surhone, Miriam T. Timpledon, Susan F. Marseken
- Genre Chemie
- EAN 9786131104077
- Format Fachbuch
- Titel Rayleigh Taylor Instability
- Herausgeber Betascript Publishing
- Anzahl Seiten 124
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