Rayleigh-Taylor 不稳定性的离散 Boltzmann LiDe-Mei ….pdf,可压流体Rayleigh-Taylor不稳定性的离散Boltzmann模拟 李德梅 赖惠林 许爱国 张广财 林传栋 甘延标 DiscreteBoltzmannsimulationofRayleigh-Taylorinstability incompressible flows LiDe-Mei LaiHui-Lin XuAi-Gu
the rayleigh-taylor instability瑞利-泰勒不稳定性 下载积分: 1000 内容提示: Vol. 62, No. 22 November 19, 2010Managed by Lockheed Martin for the National Nuclear Security AdministrationBioenergy R&D upswingWork led by Rajiv Bharadwaj andAarthi Chandrasekaran, performed atthe Joint Bio Energy Institute ...
Numerical calculations have been performed to see the effects of various parameters on the normalized growth rate of Rayleigh-Taylor instability.(For more information,please refer to the PDF.)Gamal Abdallah Hoshoudy现代物理(英文)Hoshoudy, G. (2014) Rayleigh-Taylor Instability of Magnetized Plasma ...
The magnetic Rayleigh–Taylor instability is a fundamental instability of many astrophysical systems, and recent observations are consistent with this instability developing in solar prominences. Prominences are cool, dense clouds of plasma that form in the solar corona that display a wide range of dy...
The Rayleigh — Taylor instability is the most probable mechanism to mix the ejecta of SN 1987A as suggested from observations. Although the gravity is negligible in the explosion, acceleration of the matter acts as an effective gravity and can be respon
Rayleigh–Taylor instability of the upper mantle and its role in intraplate orogeny We explore the possibility that intraplate orogeny is the result of gravitational instability of the mantle lithosphere beneath the orogenic zone. We use a... EA Neil,GA Houseman - 《Geophysical Journal of the Roya...
Growth rates of the Rayleigh-Taylor instability in foils accelerated with a laser beam smoothed by induced spatial incoherence were measured and compared with hydrodynamic code simulations. Modes with 150- and 100-μm wavelengths grew at predicted rates. However, no growth was experimentally observed ...
Rayleigh–Taylor (RT) instability指的是界面的不稳定性,重的流体向轻的流体转移。 The Rayleigh–Taylor (RT) instability describes the destabilization of the interface separating stratified fluids under the action of a gravitative acceleration directed from the heavier ...
Encyclopedia of Microfluidics & NanofluidicsMolnar, P., G. A. Houseman, G.A., 2013., Rayleigh-Taylor instability, lithospheric dynamics, surface topography at convergent mountain belts, and gravity anomalies, J. Geophys. Res. Solid Earth 118, 2544-2557....
The purpose of this paper is to prove that linearly unstable modes for Rayleigh–Taylor instabilities give birth to nonlinear instabilities for the full nonlinear system. The main ingredient is a general instability theorem in an analytic framework which enables us to go from linear to nonlinear ...