Analytic approach to nonlinear hydrodynamic instabilities driven by time-dependent accelerations.

نویسنده

  • Karnig O Mikaelian
چکیده

We extend our earlier model for Rayleigh-Taylor and Richtmyer-Meshkov instabilities to the more general class of hydrodynamic instabilities driven by a time-dependent acceleration g(t). Explicit analytic solutions for linear as well as nonlinear amplitudes are obtained for several g(t)s by solving a Schrödinger-like equation d(2)eta/dt(2)-g(t)kAeta=0, where A is the Atwood number and k is the wave number of the perturbation amplitude eta(t). In our model a simple transformation k-->k(L) and A-->A(L) connects the linear to the nonlinear amplitudes: eta(nonlinear)(k,A) approximately (1/k(L))ln eta(linear)(k(L),A(L)). The model is found to be in very good agreement with direct numerical simulations. Bubble amplitudes for a variety of accelerations are seen to scale with s defined by s=integral(square root of [g(t)]dt), while spike amplitudes prefer scaling with displacement Deltax=integral[integralg(t)dt]dt.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Nanoparticle assembly via the dewetting of patterned thin metal lines: understanding the instability mechanisms.

Nanosecond pulsed laser heating was used to control the assembly of spatially correlated nanoparticles from lithographically patterned pseudo-one-dimensional nickel lines. The evolution of the nickel line instabilities and nanoparticle formation with a correlated size and spacing was observed after a series of laser pulses. To understand the instabilities that direct the nanoparticle assembly, ...

متن کامل

Nonlinear Evolution of the Rayleigh-Taylor and Richtmyer-Meshkov Instabilities

Scaled experiments on the nonlinear evolution of the RayleighTaylor (RT) and Richtmyer-Meshkov (RM) instabilities are described under a variety, of conditions that occur in nature. At high Reynolds number, the mixi,ng layer grows self-similarly aiAgt* for a constant acceleration (g), and as a power law t*’ 1 for impulsive accelerations US(t) at low and high Mach numbers. The growth coefficients...

متن کامل

Self-Gravity Driven Instabilities of Interfaces in the ISM

In order to understand star formation it is important to understand the dynamics of atomic and molecular clouds in the interstellar medium (ISM). Nonlinear hydrodynamic flows are a key component to the ISM. One route by which nonlinear flows arise is the onset and evolution of interfacial instabilities. Interfacial instabilities act to modify the interface between gas components at different de...

متن کامل

Nonlinear Dynamics and Pattern Formation1

The objectives of our research are to improve our understanding of the mechanisms underlying the formation of complex spatio-temporal patterns in systems that are driven outside of thermodynamic equilibrium, to characterize the macroscopic properties of such states, and to apply the methodology to situations of interest in fluid physics and engineering. Current research focuses on pattern forma...

متن کامل

Nonlinear Theory of Laser Imprint, Richtmyer-Meshkov and Rayleigh-Taylor Instabilities

Implosion process in laser fusion can be divided into three phases: start-up, acceleration and stagnation phases and various hydrodynamic instabilities appear in each phase. Analytical models are developed to study nonlinear evolutions of the hydrodynamic instabilities in these phases, and compared with multi-dimensional simulations. We mainly discuss the formation of double spiral structures c...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:
  • Physical review. E, Statistical, nonlinear, and soft matter physics

دوره 81 1 Pt 2  شماره 

صفحات  -

تاریخ انتشار 2010