Hydrodynamic Instabilities And Turbulence:Rayleigh–taylor, Richtmyer–meshkov, And Kelvin–helmholtz Mixing
— 水动力不稳定性和湍流:雷利-泰勒、里希特米尔-梅什科夫和开尔文-赫尔姆霍兹混合效应
— Ye Zhou
- 中图分类 :O3
- 语种:ENG
- 出版信息:Cambridge University Press 2024.02.01 697页
- 装帧:精装 GBP150.0
- I S B N:9781108489645
- 数量:
内容简介
本书提供了前沿研究和应用方面的见解,填补了自60多年前来自该领域出现的出版空白。举例说明一些不稳定性在惯性约束聚变、反应和爆炸流、日珥、电离层流动和超新星等不同背景下发挥的关键作用。结合最新的理论,计算和实验结果,概述了核心概念和方程,随后详细描述了复杂和湍流流动。解释了稳定机制、旋转、磁场和随时间变化的加速度对水动力不稳定性演化的影响。这本书适用于本科生以及研究生,同时也是研究人员的权威参考书。
章节内容
Part I. Fundamentals: 1. A first glimpse of RT, RM & KH instabilities; 2. The linear stage for asingle mode; 3. The nonlinear stage for a single mode; 4. Multimode instabilities: linear and nonlinear regimes; 5. Global features from the lens of integrated mixing measurements; 6.Internal dynamics from the lens of statistical mixing measurements; 7. Elementary aspects of turbulent flows; 8. Transition to turbulence; Part II. Hydrodynamics of Complex Flows: 9.Influence of initial conditions; 10. Flow properties; 11. Rotation and time-dependent acceleration;12. Direction, strength, and shape of incident shock waves; 13. Reshock and multi-shocks; 14.Combined instabilities; 15. Geometrical configurations; 16. Convergent/divergent geometry; 17.Magnetohydrodynamic fluid instabilities; Part III. From the Microscopic to Cosmic Scales: 18.High energy density physics; 19. Inertial confinement fusion implosion;
20. Laboratory applications; 21. Astrophysical and space applications; 22. Mix models; 23. Numerical simulations of mixing; 24. Does 2D turbulence resemble 3D turbulence? References; Index.
20. Laboratory applications; 21. Astrophysical and space applications; 22. Mix models; 23. Numerical simulations of mixing; 24. Does 2D turbulence resemble 3D turbulence? References; Index.
学术水平:graduate students, academic researchers
读者群:mathematics, theoretical computer science