- rayleigh taylor stability
- 瑞利 泰勒稳定性
English-Chinese dictionary of mechanical engineering (英汉机械工程大词典). 2013.
rayleigh taylor stability
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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
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
Mechanism of sonoluminescence — Sonoluminescence is a phenomenon that occurs when a small gas bubble is acoustically suspended and periodically driven in a liquid solution at ultrasonic frequencies, resulting in bubble collapse, cavitation, and light emission. The thermal… … 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
Fluid dynamics — Continuum mechanics … Wikipedia
Sonoluminescence — is the emission of short bursts of light from imploding bubbles in a liquid when excited by sound.HistoryThe effect was first discovered at the University of Cologne in 1934 as a result of work on sonar. H. Frenzel and H. Schultes put an… … Wikipedia
Магниторотационная неустойчивость — Механика сплошных сред … Википедия
Магнитноротационная неустойчивость — Магниторотационная неустойчивость (МРН) это неустойчивость проводящей жидкости, вращающейся в магнитном поле. Устойчивость вращающейся жидкости без магнитного поля изучалась Куэттом (англ.) (Couette, 1890)[1], Маллоком (Mallock, 1896)[2], Рэлеем… … Википедия
Humphreys-Davidson-Grenze — Die Humphreys Davidson Grenze ist die empirisch bestimmte maximale Leuchtkraft, in der ein Stern im hydrostatischen Gleichgewicht existieren kann. Sie wurde erstmals von den amerikanischen Astronomen R. M. Humphreys und K. Davidsons im Jahre 1979 … Deutsch Wikipedia
