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arXiv 1010.1189physics.plasm-ph
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Rayleigh-Taylor、Kelvin-Helmholtz和Richtmyer-Meshkov不稳定性组合action引起的非线性双流体界面结构的发展:斜激波

Development of nonlinear two fluid interfacial structures by combined action of Rayleigh-Taylor, Kelvin-Helmholtz and Richtmyer-Meshkov instabilities:Oblique shock

M. R. Gupta, Labakanta Mandal, Sourav Roy, Rahul Banerjee, Manoranjan Khan

摘要:

研究了由于Rayleigh-Taylor不稳定性和Kelvin-Helmholtz不稳定性的联合作用或由于Richtmyer-Meshkov不稳定性和Kelvin-Helmholtz不稳定性的联合作用而产生的气泡和尖峰等两种流体界面结构的非线性演化。使用雷泽模型的分析表达式的渐近值的组合增长率在这两种情况下获得的尖峰和泡沫。然而,如果上覆流体的密度较低,则界面扰动以不同的方式表现。取决于与开尔文-亥姆霍兹不稳定性相关的速度剪切的大小,气泡和尖峰振幅可能同时单调增长(不稳定性)或随时间振荡,或者可能发生这样的情况,即当尖峰变陡时,气泡倾向于波动。在斜激波的情况下,由于激波的法向分量引起的Richtmyer-Meshkov不稳定性和由于其平行分量在两流体界面上产生的速度剪切引起的Kelvin-Helmholtz不稳定性的联合作用,不稳定性增长率--而不是表现为正激波的$t \rightarrow \infty$那样的$1/t$,渐近地趋向于穗峰值高度生长速度$\sim \sqrt{\frac{5(1+A_{T})}{16(1-A_{T})}(Δv)^2}$,其中$Δv $是速度切变,$A_T$是阿特伍德数。这种结果的含义与生成的尖峰流体射流在天体物理方面进行了讨论。

英文摘要:

The nonlinear evolution of two fluid interfacial structures like bubbles and spikes arising due to the combined action of Rayleigh-Taylor and Kelvin-Helmholtz instability or due to that of Richtmyer-Meshkov and Kelvin-Helmholtz instability resulting from oblique shock is investigated. Using Layzer's model analytic expressions for the asymptotic value of the combined growth rate are obtained in both cases for spikes and bubbles. However, if the overlying fluid is of lower density the interface perturbation behaves in different ways. Depending on the magnitude of the velocity shear associated with Kelvin-Helmholtz instability both the bubble and spike amplitude may simultaneously grow monotonically (instability) or oscillate with time or it may so happen that while this spike steepens the bubble tends to undulate. In case of an oblique shock which causes combined action of Richtmyer-Meshkov instability arising due to the normal component of the shock and Kelvin Helmholtz instability through creation of velocity shear at the two fluid interface due to its parallel component, the instability growth rate-instead of behaving as $1/t$ as $t \rightarrow \infty$ for normal shock, tends asymptotically to a spike peak height growth velocity $\sim \sqrt{\frac{5(1+A_{T})}{16(1-A_{T})}(Δv)^2}$ where $Δv $ is the velocity shear and $A_T$ is the Atwood number. Implication of such result in connection with generation of spiky fluid jets in astrophysical context is discussed.

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