Stratified flows are characterized by density variations in fluids, often due to temperature or salinity gradients. These flows exhibit layered structures, with denser fluid underlying lighter fluid, leading to stable configurations. Stratification significantly influences fluid dynamics, suppressing vertical mixing and altering wave and turbulence propagation.
Density variations in stratified flows can arise from temperature differences or solute concentration variations. In the atmosphere, temperature gradients primarily cause density variations, while in the ocean, both temperature and salinity influence density. Understanding these variations is crucial for analyzing fluid behavior in various environmental systems.
Characteristics of stratified flows
Stratified flows are characterized by the presence of density variations in the fluid, often due to temperature or salinity gradients
These flows exhibit a layered structure, with denser fluid underlying lighter fluid, leading to a stable configuration
Stratification can significantly influence the dynamics of fluid motion, suppressing vertical mixing and altering the propagation of waves and turbulence
Density variations in stratified flows
Density variations in stratified flows can arise from temperature differences () or variations in solute concentration ()
In the atmosphere, density variations are primarily caused by temperature gradients, with cooler, denser air near the Earth's surface and warmer, lighter air aloft
In the ocean, density variations are influenced by both temperature and salinity, with colder, saltier water being denser than warmer, fresher water
Stability of stratified flows
Stable stratification
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occurs when the density of the fluid increases with depth, leading to a configuration where lighter fluid overlies denser fluid
In this case, the force acts to restore any vertical displacements, suppressing vertical mixing and turbulence
Examples of stable stratification include the thermocline in the ocean and the troposphere in the atmosphere
Unstable stratification
arises when the density of the fluid decreases with depth, resulting in a situation where denser fluid overlies lighter fluid
This configuration is prone to convective instabilities, as any vertical perturbations will be amplified by the buoyancy force
Examples of unstable stratification include the convective boundary layer in the atmosphere and the mixed layer in the ocean
Neutral stratification
refers to a situation where the density of the fluid remains constant with depth
In this case, the buoyancy force does not influence vertical motions, and the flow behaves similarly to homogeneous turbulence
Neutral stratification can occur in well-mixed regions, such as the surface mixed layer in the ocean or the atmospheric boundary layer under strong wind conditions
Internal waves
Characteristics of internal waves
are that propagate within the interior of a stratified fluid, rather than on the free surface
These waves are driven by buoyancy forces and can have much larger amplitudes and slower propagation speeds compared to surface waves
Internal waves are characterized by their frequency, wavenumber, and vertical structure, which depend on the and background flow conditions
Generation of internal waves
Internal waves can be generated by various mechanisms, including flow over topography, wind stress on the ocean surface, and tidal forcing
When a stratified fluid encounters an obstacle (seamount), the flow is deflected vertically, generating internal waves that propagate away from the topography
Wind stress can generate internal waves through resonant interactions with surface waves or by directly forcing vertical motions in the upper ocean
Propagation of internal waves
Internal waves propagate along surfaces of constant density (isopycnals) in a stratified fluid
The propagation direction and speed of internal waves depend on the frequency, wavenumber, and stratification profile
As internal waves propagate, they can interact with other waves, leading to energy transfers, wave breaking, and mixing
Mixing in stratified flows
Turbulent mixing
Turbulent mixing in stratified flows is driven by shear instabilities and
When the shear in the flow exceeds a critical threshold (), can develop, leading to the formation of turbulent billows and enhanced mixing
Breaking internal waves can also generate turbulence and mixing, particularly in regions of high wave activity or near critical layers
Molecular diffusion
is the transport of heat, salt, or other scalars due to random molecular motions
In stratified flows, molecular diffusion is often much weaker than turbulent mixing, but it can be important in regions of weak turbulence or strong gradients
is a special case where the different molecular diffusivities of heat and salt can lead to enhanced mixing and the formation of staircase-like density profiles
Entrainment and detrainment
refers to the incorporation of fluid from one layer into another, typically from a less turbulent to a more turbulent region
Detrainment is the opposite process, where fluid is expelled from a turbulent region into a less turbulent one
In stratified flows, entrainment and detrainment can occur across density interfaces, leading to the exchange of mass, momentum, and scalars between layers
Stratified flow regimes
Layered flows
are characterized by the presence of distinct layers with sharp density interfaces separating them
These flows can arise from the interaction of different water masses (estuaries), or from the effects of surface heating or cooling (thermocline)
Layered flows often exhibit reduced vertical mixing and enhanced horizontal dispersion, as well as the formation of internal waves and hydraulic jumps at the interfaces
Continuous stratification
Continuously stratified flows have a smooth density profile, with no distinct layers or interfaces
These flows are common in the ocean interior and the upper atmosphere, where density varies gradually with depth
supports the propagation of internal waves and can lead to the formation of thin layers of enhanced mixing or biological activity
Froude number in stratified flows
The is a dimensionless parameter that compares the inertial forces to the buoyancy forces in a stratified flow
It is defined as Fr=U/(NH), where U is a characteristic velocity, N is the buoyancy frequency, and H is a characteristic length scale
The Froude number is used to characterize the flow regime and the importance of stratification effects
For Fr<<1, the flow is strongly influenced by stratification, and internal waves can propagate freely
For Fr>>1, the flow is dominated by inertial effects, and stratification has a weak influence on the dynamics
Modeling stratified flows
Analytical models
Analytical models of stratified flows are based on simplified equations that capture the essential physics of the problem
These models often assume idealized geometries, linear density profiles, and small perturbations to the background flow
Examples of analytical models include the for linear internal waves and the for nonlinear internal solitary waves
Numerical models
Numerical models are used to simulate stratified flows in more complex geometries and with realistic forcing and boundary conditions
These models solve the Navier-Stokes equations with an equation of state that relates density to temperature and salinity
Numerical models can capture a wide range of stratified flow phenomena, including internal waves, turbulence, and mixing
Examples of numerical models for stratified flows include the and the
Applications of stratified flows
Atmospheric stratification
Atmospheric stratification plays a crucial role in weather and climate dynamics
The stability of the atmospheric boundary layer influences the formation of clouds, the dispersion of pollutants, and the intensity of turbulence
Internal waves in the atmosphere (gravity waves) can transport momentum and energy over large distances and contribute to the forcing of the global circulation
Oceanic stratification
Oceanic stratification is important for the global climate system, as it controls the storage and transport of heat, carbon, and nutrients
The ocean's density structure influences the formation and circulation of water masses, as well as the propagation of internal waves and tides
Mixing in the stratified ocean interior is crucial for maintaining the global overturning circulation and the distribution of biogeochemical tracers
Environmental fluid dynamics
Stratified flows are relevant to a wide range of environmental fluid dynamics problems, such as the dispersion of pollutants in the atmosphere and ocean
The stability of the atmospheric boundary layer affects the transport and mixing of air pollutants, with stable conditions leading to reduced dispersion and higher concentrations
In the ocean, stratification can influence the fate and transport of oil spills, as well as the dispersion of nutrients and biological productivity
Experimental techniques for stratified flows
Density measurements
Density measurements in stratified flows can be performed using various techniques, such as conductivity-temperature-depth (CTD) sensors, which measure the electrical conductivity and temperature of the fluid to infer density
Other methods include the use of density floats (drift along surfaces of constant density) or the analysis of refractive index variations using optical techniques (schlieren)
Velocity measurements
Velocity measurements in stratified flows can be obtained using acoustic Doppler current profilers (ADCPs), which use the Doppler shift of sound waves to measure the velocity profile
Other techniques include particle image velocimetry (PIV), which tracks the motion of tracer particles in the fluid, and laser Doppler velocimetry (LDV), which measures the velocity at a point based on the Doppler shift of scattered laser light
Flow visualization
Flow visualization techniques are used to qualitatively observe the structure and dynamics of stratified flows
Dye tracers can be injected into the fluid to highlight the motion of fluid parcels and the formation of internal waves or turbulent structures
Shadowgraph and schlieren imaging techniques can be used to visualize density variations in the fluid based on changes in the refractive index
Mathematical description of stratified flows
Governing equations
The governing equations for stratified flows are the Navier-Stokes equations, which describe the conservation of mass, momentum, and energy in the fluid
The equations are coupled with an equation of state that relates density to temperature and salinity, such as the linear equation of state: ρ=ρ0(1−α(T−T0)+β(S−S0))
The Boussinesq approximation is often used in stratified flows, which assumes that density variations are small and only affect the buoyancy term in the momentum equation
Boundary conditions
Boundary conditions for stratified flows depend on the specific problem and geometry considered
At the free surface, the boundary conditions typically include a wind stress condition for the momentum equation and a heat and salt flux condition for the scalar equations
At solid boundaries (bottom), no-slip and no-flux conditions are often imposed, although slip or flux conditions can be used in some cases
Initial conditions
Initial conditions for stratified flows specify the density and velocity fields at the start of the simulation or experiment
These conditions can be based on observations, analytical solutions, or previous numerical simulations
The choice of initial conditions can strongly influence the subsequent evolution of the flow, particularly in the case of instabilities or transient phenomena