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Laminar and turbulent flows are fundamental concepts in fluid dynamics. They describe how fluids behave under different conditions, with characterized by smooth, parallel layers and by chaotic, irregular motion.

The is a key factor in determining flow regime. It's a dimensionless number that predicts whether flow will be laminar or turbulent based on fluid properties, velocity, and system geometry. Understanding these concepts is crucial for engineering applications.

Laminar vs turbulent flow

  • Laminar flow characterized by smooth, parallel layers of fluid with no mixing between layers
  • Turbulent flow characterized by chaotic, irregular motion with mixing between layers
  • Laminar flow occurs at low velocities and in small diameter pipes, while turbulent flow occurs at high velocities and in large diameter pipes

Reynolds number

  • Dimensionless number that predicts the flow regime based on the ratio of inertial forces to viscous forces
  • Defined as Re=ρvDμRe = \frac{\rho v D}{\mu}, where ρ\rho is density, vv is velocity, DD is characteristic length (pipe diameter), and μ\mu is dynamic viscosity
  • Higher Reynolds numbers indicate a greater tendency for turbulent flow, while lower values indicate laminar flow

Critical Reynolds number

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  • The Reynolds number at which the flow occurs
  • For pipe flow, the is approximately 2300
  • Flow below the critical Reynolds number is laminar, while flow above it is turbulent

Predicting flow regime

  • The flow regime (laminar or turbulent) can be predicted using the Reynolds number
  • Laminar flow occurs when Re<RecriticalRe < Re_{critical}, while turbulent flow occurs when Re>RecriticalRe > Re_{critical}
  • The critical Reynolds number depends on the geometry and surface roughness of the system

Characteristics of laminar flow

  • Fluid particles move in smooth, parallel layers with no mixing between layers
  • is parabolic, with the highest velocity at the center and zero velocity at the walls
  • is directly proportional to the fluid velocity and inversely proportional to the pipe diameter

Velocity profile

  • In laminar flow, the velocity profile is parabolic, with the highest velocity at the center and zero velocity at the walls
  • The velocity profile is described by the : v(r)=ΔP4μL(R2r2)v(r) = \frac{\Delta P}{4\mu L}(R^2 - r^2), where ΔP\Delta P is the pressure drop, LL is the pipe length, RR is the pipe radius, and rr is the radial position
  • The average velocity is half of the maximum velocity at the center

Pressure drop

  • In laminar flow, the pressure drop is directly proportional to the fluid velocity and inversely proportional to the pipe diameter
  • The pressure drop is described by the Hagen-Poiseuille equation: ΔP=8μLQπR4\Delta P = \frac{8\mu LQ}{\pi R^4}, where QQ is the volumetric flow rate
  • Pressure drop in laminar flow is lower than in turbulent flow for the same flow rate

Entrance length

  • The is the distance from the pipe inlet where the velocity profile is fully developed
  • For laminar flow, the entrance length is approximately Le=0.06ReDL_e = 0.06 Re D
  • Flow in the entrance region is not fully developed and has a higher pressure drop than fully developed flow

Characteristics of turbulent flow

  • Fluid particles move in a chaotic, irregular manner with mixing between layers
  • Velocity fluctuates in both magnitude and direction
  • Pressure drop is proportional to the square of the fluid velocity and inversely proportional to the pipe diameter

Velocity fluctuations

  • In turbulent flow, the velocity fluctuates in both magnitude and direction
  • are caused by , which are rotating structures of fluid
  • The root-mean-square (RMS) of the velocity fluctuations is a measure of the turbulence intensity

Turbulent eddies

  • Turbulent eddies are rotating structures of fluid that cause mixing and velocity fluctuations
  • Eddies range in size from the largest (limited by the system geometry) to the smallest (determined by viscosity)
  • Energy is transferred from larger eddies to smaller eddies in a process called the energy cascade

Turbulent boundary layer

  • In turbulent flow over a surface, a develops
  • The turbulent boundary layer consists of a viscous sublayer (near the wall), a buffer layer, and a fully turbulent region
  • The thickness of the turbulent boundary layer increases with distance from the leading edge

Transition from laminar to turbulent

  • The transition from laminar to turbulent flow occurs when the Reynolds number exceeds the critical value
  • The transition is not instantaneous but occurs over a certain distance called the transition region
  • In the transition region, the flow alternates between laminar and turbulent states

Transition mechanisms

  • The transition from laminar to turbulent flow can occur through different mechanisms
  • Natural transition occurs due to the amplification of small disturbances in the flow
  • Bypass transition occurs when large disturbances (such as surface roughness) directly trigger turbulence
  • Separated flow transition occurs when the flow separates from the surface and becomes turbulent

Factors affecting transition

  • The transition from laminar to turbulent flow is affected by various factors
  • Surface roughness promotes transition by introducing disturbances into the flow
  • Pressure gradient affects transition, with adverse pressure gradients promoting transition and favorable pressure gradients delaying it
  • Freestream turbulence (turbulence in the flow upstream of the surface) can trigger bypass transition

Friction factors

  • The is a dimensionless number that relates the pressure drop to the flow velocity and pipe diameter
  • Different expressions are used for the friction factor in laminar and turbulent flow
  • The friction factor depends on the Reynolds number and the relative roughness of the pipe surface

Laminar friction factor

  • In laminar flow, the friction factor is inversely proportional to the Reynolds number
  • The is given by f=64Ref = \frac{64}{Re}
  • This expression is valid for fully developed laminar flow in circular pipes

Turbulent friction factor

  • In turbulent flow, the friction factor depends on both the Reynolds number and the relative roughness of the pipe surface
  • The can be determined using empirical correlations, such as the Colebrook equation or the
  • The Colebrook equation is an implicit equation that requires iterative solution: 1f=2.0log10(ϵ/D3.7+2.51Ref)\frac{1}{\sqrt{f}} = -2.0 \log_{10} \left(\frac{\epsilon/D}{3.7} + \frac{2.51}{Re\sqrt{f}}\right), where ϵ/D\epsilon/D is the relative roughness

Moody diagram

  • The Moody diagram is a graphical representation of the friction factor as a function of Reynolds number and relative roughness
  • It allows the friction factor to be determined without the need for iterative calculations
  • The diagram has different curves for different values of relative roughness, with smooth pipes represented by the lowest curve

Flow in pipes

  • can be laminar or turbulent, depending on the Reynolds number
  • The pressure drop and velocity profile differ between laminar and
  • in pipes are caused by friction and minor losses (such as bends and valves)

Laminar pipe flow

  • In , the velocity profile is parabolic, with the highest velocity at the center and zero velocity at the walls
  • The pressure drop is directly proportional to the fluid velocity and inversely proportional to the pipe diameter
  • The Hagen-Poiseuille equation can be used to calculate the pressure drop and velocity profile

Turbulent pipe flow

  • In turbulent pipe flow, the velocity profile is flatter than in laminar flow, with a more uniform velocity distribution
  • The pressure drop is proportional to the square of the fluid velocity and inversely proportional to the pipe diameter
  • Empirical correlations (such as the Colebrook equation) or the Moody diagram can be used to determine the friction factor

Pressure losses

  • Pressure losses in pipes are caused by friction and minor losses
  • Friction losses are due to the shear stress between the fluid and the pipe wall and can be calculated using the : hf=fLDv22gh_f = f \frac{L}{D} \frac{v^2}{2g}, where hfh_f is the head loss due to friction, ff is the friction factor, LL is the pipe length, DD is the pipe diameter, vv is the fluid velocity, and gg is the acceleration due to gravity
  • Minor losses are caused by flow disturbances (such as bends, valves, and contractions) and can be calculated using loss coefficients: hm=Kv22gh_m = K \frac{v^2}{2g}, where hmh_m is the head loss due to minor losses and KK is the loss coefficient

Flow over surfaces

  • can be laminar or turbulent, depending on the Reynolds number and surface geometry
  • The behavior of the flow near the surface is described by boundary layer theory
  • Flow separation can occur when the boundary layer encounters an adverse pressure gradient

Laminar boundary layer

  • In laminar flow over a surface, a develops
  • The laminar boundary layer is characterized by smooth, parallel streamlines
  • The thickness of the laminar boundary layer increases with distance from the leading edge, as described by the Blasius solution

Turbulent boundary layer

  • In turbulent flow over a surface, a turbulent boundary layer develops
  • The turbulent boundary layer is characterized by chaotic, irregular motion and mixing
  • The thickness of the turbulent boundary layer increases more rapidly than the laminar boundary layer

Separation and reattachment

  • Flow separation occurs when the boundary layer encounters an adverse pressure gradient and detaches from the surface
  • Separation can be caused by a change in surface geometry (such as a sharp corner) or by an adverse pressure gradient imposed by the external flow
  • After separation, the flow may reattach to the surface, forming a separation bubble
  • Flow separation can lead to increased drag, reduced lift, and unsteady flow phenomena (such as vortex shedding)

Turbulence modeling

  • is the process of approximating the effects of turbulence in fluid flow simulations
  • of turbulence is computationally expensive, so turbulence models are used to reduce the computational cost
  • Turbulence models can be classified as models, models, or hybrid RANS-LES models

Reynolds-averaged Navier-Stokes (RANS)

  • RANS models solve the time-averaged Navier-Stokes equations, with the effects of turbulence represented by additional terms (Reynolds stresses)
  • The Reynolds stresses are modeled using turbulence models, such as the k-epsilon model or the k-omega model
  • RANS models are computationally efficient but may not capture all the details of turbulent flow

Large eddy simulation (LES)

  • LES models directly simulate the large-scale turbulent eddies and model the effects of smaller-scale eddies
  • The Navier-Stokes equations are filtered to remove the small-scale eddies, and a subgrid-scale model is used to represent their effects
  • LES models are more accurate than RANS models but are computationally more expensive

Direct numerical simulation (DNS)

  • DNS directly solves the Navier-Stokes equations without any turbulence modeling
  • All scales of turbulent motion are resolved, from the largest eddies to the smallest dissipative scales
  • DNS is the most accurate method for simulating turbulent flow but is computationally very expensive and limited to low Reynolds numbers

Applications of laminar and turbulent flows

  • Laminar and turbulent flows have various applications in engineering and natural systems
  • The choice between laminar and turbulent flow depends on the specific requirements of the application
  • Laminar flow is often preferred for applications requiring low mixing or high precision, while turbulent flow is preferred for applications requiring high mixing or

Heat transfer

  • Turbulent flow enhances heat transfer compared to laminar flow due to the increased mixing and transport of heat
  • In heat exchangers, turbulent flow is often used to increase the heat transfer coefficient and improve efficiency
  • Laminar flow may be used in applications where a uniform temperature distribution is required, such as in certain electronic cooling systems

Mass transfer

  • Turbulent flow enhances compared to laminar flow due to the increased mixing and transport of species
  • In chemical reactors, turbulent flow is often used to promote mixing and increase the reaction rate
  • Laminar flow may be used in applications where a controlled and uniform distribution of species is required, such as in certain drug delivery systems

Mixing and dispersion

  • Turbulent flow promotes of species due to the chaotic motion and increased diffusivity
  • In environmental systems (such as rivers and atmospheric flows), turbulent flow is responsible for the mixing and dispersion of pollutants
  • Laminar flow may be used in applications where mixing needs to be minimized, such as in certain microfluidic devices or in the production of composite materials
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© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.

© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.
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