Nonlinear Saturation Amplitude in Classical Planar Richtmyer–Meshkov Instability
The classical planar Richtmyer–Meshkov instability(RMI) at a fluid interface supported by a constant pressure is investigated by a formal perturbation expansion up to the third order,and then according to definition of nonlinear saturation amplitude(NSA) in Rayleigh–Taylor instability(RTI),the NSA i...
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| Published in | Communications in theoretical physics Vol. 65; no. 4; pp. 523 - 526 |
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| Main Author | |
| Format | Journal Article |
| Language | English |
| Published |
01.04.2016
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| Subjects | |
| Online Access | Get full text |
| ISSN | 0253-6102 1572-9494 |
| DOI | 10.1088/0253-6102/65/4/523 |
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| Abstract | The classical planar Richtmyer–Meshkov instability(RMI) at a fluid interface supported by a constant pressure is investigated by a formal perturbation expansion up to the third order,and then according to definition of nonlinear saturation amplitude(NSA) in Rayleigh–Taylor instability(RTI),the NSA in planar RMI is obtained explicitly.It is found that the NSA in planar RMI is affected by the initial perturbation wavelength and the initial amplitude of the interface,while the effect of the initial amplitude of the interface on the NSA is less than that of the initial perturbation wavelength.Without marginal influence of the initial amplitude,the NSA increases linearly with wavelength.The NSA normalized by the wavelength in planar RMI is about 0.11,larger than that corresponding to RTI. |
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| AbstractList | The classical planar Richtmyer-Meshkov instability (RMI) at a fluid interface supported by a constant pressure is investigated by a formal perturbation expansion up to the third order, and then according to definition of nonlinear saturation amplitude (NSA) in Rayleigh-Taylor instability (RTI), the NSA in planar RMI is obtained explicitly. It is found that the NSA in planar RMI is affected by the initial perturbation wavelength and the initial amplitude of the interface, while the effect of the initial amplitude of the interface on the NSA is less than that of the initial perturbation wavelength. Without marginal influence of the initial amplitude, the NSA increases linearly with wavelength. The NSA normalized by the wavelength in planar RMI is about 0.11, larger than that corresponding to RTI. The classical planar Richtmyer–Meshkov instability(RMI) at a fluid interface supported by a constant pressure is investigated by a formal perturbation expansion up to the third order,and then according to definition of nonlinear saturation amplitude(NSA) in Rayleigh–Taylor instability(RTI),the NSA in planar RMI is obtained explicitly.It is found that the NSA in planar RMI is affected by the initial perturbation wavelength and the initial amplitude of the interface,while the effect of the initial amplitude of the interface on the NSA is less than that of the initial perturbation wavelength.Without marginal influence of the initial amplitude,the NSA increases linearly with wavelength.The NSA normalized by the wavelength in planar RMI is about 0.11,larger than that corresponding to RTI. |
| Author | 刘万海 王翔 蒋宏彬 马文芳 |
| AuthorAffiliation | Research Center of Computational Physics, Mianyang Normal University, Mianyang 621000, China School of Bailie Engineering and Technology, Lanzhou City University, Lanzhou 730070, China |
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| Cites_doi | 10.1007/BF01015969 10.1002/cpa.3160130207 10.1103/PhysRevE.63.056303 10.1098/rspa.1950.0052 10.1063/1.871209 10.1017/S002211209500379X 10.1103/PhysRevLett.74.534 10.1063/1.868245 10.1063/1.873491 10.1103/PhysRevLett.71.2903 10.1063/1.4819765 10.1103/PhysRevE.58.4548 10.1103/PhysRevLett.71.3473 10.1063/1.1362529 10.1103/PhysRevE.67.026301 10.1103/PhysRevE.87.013006 10.7498/aps.52.1688 10.1063/1.872341 10.1017/S002211208800045X 10.1063/1.868391 10.1063/1.869202 10.1063/1.859603 10.1103/PhysRevE.69.036703 10.1063/1.3702063 |
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| Notes | Wan-Hai Liu ,Xiang Wang , Hong-Bin Jiang,Wen-Fang Ma(1Research Center of Computational Physics, Mianyang Normal University, Mianyang 621000, China ;2School of Bailie Engineering and Technology, Lanzhou City University, Lanzhou 730070, China) Richtmyer–Meshkov instability nonlinear saturation amplitude perturbation expansion The classical planar Richtmyer–Meshkov instability(RMI) at a fluid interface supported by a constant pressure is investigated by a formal perturbation expansion up to the third order,and then according to definition of nonlinear saturation amplitude(NSA) in Rayleigh–Taylor instability(RTI),the NSA in planar RMI is obtained explicitly.It is found that the NSA in planar RMI is affected by the initial perturbation wavelength and the initial amplitude of the interface,while the effect of the initial amplitude of the interface on the NSA is less than that of the initial perturbation wavelength.Without marginal influence of the initial amplitude,the NSA increases linearly with wavelength.The NSA normalized by the wavelength in planar RMI is about 0.11,larger than that corresponding to RTI. 11-2592/O3 ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
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| References | 22 23 24 25 Wang L.F. (11) 2010; 90 26 27 28 Benjamin R. (14) 1993 Rayleigh L. (3) 1883; 14 10 15 16 17 18 19 1 2 Ye W.H. (12) 2003; 52 4 5 6 7 8 9 Aleshin A.N. (13) 1990; 35 20 21 |
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| Snippet | The classical planar Richtmyer–Meshkov instability(RMI) at a fluid interface supported by a constant pressure is investigated by a formal perturbation... The classical planar Richtmyer-Meshkov instability (RMI) at a fluid interface supported by a constant pressure is investigated by a formal perturbation... |
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| SubjectTerms | Amplitudes Constants Instability Nonlinearity NSA Perturbation RMI Saturation Stability Wavelengths 不稳定性 初始扰动 幅度 平面 流体界面 非线性饱和 |
| Title | Nonlinear Saturation Amplitude in Classical Planar Richtmyer–Meshkov Instability |
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