- rayleigh taylor instability
- 瑞利 泰勒不稳定性
English-Chinese dictionary of mechanical engineering (英汉机械工程大词典). 2013.
rayleigh taylor instability
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Rayleigh–Taylor instability — 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. [citation… … Wikipedia
Instabilité de Rayleigh–Taylor — Instabilité de Rayleigh Taylor Manifestation de l instabilité de Rayleigh–Taylor dans la nébuleuse du Crabe. L’instabilité de Rayleigh–Taylor, nommée en hommage aux physiciens britanniques Lord Rayleigh et G. I. Taylor, est une instabilité de… … Wikipédia en Français
Instabilité de Rayleigh-Taylor — Manifestation de l instabilité de Rayleigh–Taylor dans la nébuleuse du Crabe. L’instabilité de Rayleigh–Taylor, nommée en hommage aux physiciens britanniques Lord Rayleigh et G. I. Taylor, est une instabilité de l’interface séparant deux fluides… … Wikipédia en Français
Inestabilidad Rayleigh-Taylor — Evidencia de IRT en la nebulosa del Cangrejo. Simulación … Wikipedia Español
Instability — [ Hydrodynamics simulation of the Rayleigh–Taylor instability [Shengtai Li, Hui Li Parallel AMR Code for Compressible MHD or HD Equations (Los Alamos National Laboratory) [http://math.lanl.gov/Research/Highlights/amrmhd.shtml] ] ] Instability in… … Wikipedia
Richtmyer-Meshkov instability — The Richtmyer Meshkov instability (RMI) occurs when an interface between fluids of differing density is impulsively accelerated, e.g. by the passage of a shock wave. The development of the instability begins with small amplitude perturbations… … Wikipedia
Plateau-Rayleigh instability — The Plateau Rayleigh instability, often just called the Rayleigh instability , explains why and how a falling stream of fluid breaks up into smaller packets with the same volume but less surface area. It is related to the Rayleigh–Taylor… … Wikipedia
Kelvin–Helmholtz instability — Numerical simulation of a temporal Kelvin–Helmholtz instability The Kelvin–Helmholtz instability, after Lord Kelvin and Hermann von Helmholtz, can occur when velocity shear is present within a continuous fluid, or when there is sufficient… … Wikipedia
John Strutt, 3rd Baron Rayleigh — Infobox Scientist name = Lord Rayleigh caption = John William Strutt, 3rd Baron Rayleigh birth date = Birth date|1842|11|12|df=yes birth place = Langford Grove, Maldon, Essex, England death date = Death date and age|1919|6|30|1842|11|12|df=yes… … Wikipedia
Geoffrey Ingram Taylor — Infobox Scientist name = Geoffrey Ingram Taylor image width = 250px caption = Sir Geoffrey Ingram Taylor birth date = 7 March 1886 birth place = St. John s Wood, London death date = 27 June 1975 death place = Cambridge residence = citizenship =… … Wikipedia
Taylor number — In fluid dynamics, the Taylor number is a dimensionless quantity that characterizes the importance of centrifugal forces or so called inertial forces due to rotation of a fluid about a vertical axis, relative to viscous forces. The typical… … Wikipedia
